CLINICAL PHARMACY IN HEMATOLOGY. SYMPTOMS AND SYNDROMES IN MAJOR DISEASES OF THE BLOOD SYSTEM. CLINICAL PHARMACOLOGY OF IRON PREPARATIONS AND OTHER ANTIANEMIC AGENTS
Hemostasis refers to the finely regulated dynamic process of maintaining fluidity of the blood, repairing vascular injury, and limiting blood loss while avoiding vessel occlusion (thrombosis) and inadequate perfusion of vital organs. Either extreme¾excessive bleeding or thrombosis¾represents a breakdown of the hemostatic mechanism. Common causes of dysregulated hemostasis include hereditary or acquired defects in the clotting mechanism and secondary effects of infection or cancer. The drugs used to limit abnormal bleeding and to inhibit thrombosis are the subjects of this chapter.
MECHANISMS OF BLOOD COAGULATION
The vascular endothelial cell layer lining blood vessels has an anticoagulant phenotype, and circulating blood platelets and clotting factors do not normally adhere to it to an appreciable extent. In the setting of vascular injury, the endothelial cell layer rapidly undergoes a series of changes resulting in a more procoagulant phenotype. Injury exposes reactive subendothelial matrix proteins such as collagen and von Willebrand factor, which results in platelet adherence and activation, and secretion and synthesis of vasoconstrictors and platelet-recruiting and activating molecules. Thus, thromboxane A2 (TXA2) is synthesized from arachadonic acid within platelets and is a platelet activator and potent vasoconstrictor. Products secreted from platelet granules include adenosine diphosphate (ADP), a powerful inducer of platelet aggregation, and serotonin (5-HT), which stimulates aggregation and vasoconstriction. Activation of platelets results in a conformational change in the aIIbbIII integrin (IIb/IIIa) receptor, enabling it to bind fibrinogen, which cross-links adjacent platelets, resulting in aggregation and formation of a platelet plug. Simultaneously, the coagulation system cascade is activated, resulting in thrombin generation and a fibrin clot, which stabilizes the platelet plug (see below). Knowledge of the hemostatic mechanism is important for diagnosis of bleeding disorders. Patients with defects in the formation of the primary platelet plug (defects in primary hemostasis, eg, platelet function defects, von Willebrand disease) typically bleed from mucosal sites (gingiva, skin, heavy menses) with injury. In contrast, patients with defects in the clotting mechanism (secondary hemostasis, eg, hemophilia A) tend to bleed into deep tissues (joints, muscle, retroperitoneum), often with no apparent inciting event, and bleeding may recur unpredictably.
Thrombus formation at the site of the damaged vascular wall
The platelet is central to normal hemostasis and thromboembolic disease, and is the target of many therapies discussed in this chapter. Platelet-rich thrombi (white thrombi) form in the high flow rate and high shear force environment of arteries. Occlusive arterial thrombi cause serious disease by producing downstream ischemia of extremities or vital organs, and can result in limb amputation or organ failure. Venous clots tend to be more fibrin-rich, contain large numbers of trapped red blood cells, and are recognized pathologically as red thrombi. Venous thrombi can cause severe swelling and pain of the affected extremity, but the most feared consequence is pulmonary embolism. This occurs when part or all of the clot breaks off from its location in the deep venous system and travels as an embolus through the right side of the heart and into the pulmonary arterial circulation. Sudden occlusion of a large pulmonary artery can cause acute right heart failure and sudden death. In addition lung ischemia or infarction will occur distal to the occluded pulmonary arterial segment. Such emboli usually arise from the deep venous system of the proximal lower extremities or pelvis. Although all thrombi are mixed, the platelet nidus dominates the arterial thrombus and the fibrin tail dominates the venous thrombus.
Blood coagulates by the transformation of soluble fibrinogen into insoluble fibrin. Several circulating proteins interact in a cascading series of limited proteolytic reactions. At each step, a clotting factor zymogen undergoes limited proteolysis and becomes an active protease (eg, factor VII is converted to factor VIIa). Each protease factor activates the next clotting factor in the sequence, culminating in the formation of thrombin (factor IIa). Several of these factors are targets for drug therapy Thrombin has a central role in hemostasis and has many functions. In clotting, thrombin proteolytically cleaves small peptides from fibrinogen, allowing fibrinogen to polymerize and form a fibrin clot. Thrombin also activates many upstream clotting factors, leading to more thrombin generation, and activates factor XIII, a transaminase that cross-links the fibrin polymer and stabilizes the clot. Thrombin is a potent platelet activator and mitogen. Thrombin also exerts anticoagulant effects by activating the protein C pathway, which attenuates the clotting response. It should therefore be apparent that the response to vascular injury is a complex and precisely modulated process that ensures that under normal circumstances, repair of vascular injury occurs without thrombosis and downstream ischemia; that is, the response is proportionate and reversible. Eventually vascular remodeling and repair occur with reversion to the quiescent resting anticoagulant endothelial cell phenotype.
Initiation of Clotting: The Tissue Factor-VIIa Complex
The main initiator of blood coagulation in vivo is the tissue factor (TF)-factor VIIa pathway. Tissue factor is a transmembrane protein ubiquitously expressed outside the vasculature, but not normally expressed in an active form within vessels. The exposure of TF on damaged endothelium or to blood that has extravasated into tissue binds TF to factor VIIa. This complex, in turn, activates factors X and IX. Factor Xa along with factor Va forms the prothrombinase complex on activated cell surfaces, which catalyzes the conversion of prothrombin (factor II) to thrombin (factor IIa). Thrombin, in turn, activates upstream clotting factors, primarily factors V, VIII, and XI, resulting in amplification of thrombin generation. The TF-factor VIIa-catalyzed activation of factor Xa is regulated by tissue factor pathway inhibitor (TFPI). Thus after initial activation of factor X to Xa by TF-VIIa, further propagation of the clot is by feedback amplification of thrombin through the intrinsic pathway factors VIII and IX (this provides an explanation of why patients with deficiency of factor VIII or IX¾hemophilia A and hemophilia B, respectively¾have a severe bleeding disorder).
It is also important to note that the coagulation mechanism in vivo does not occur in solution, but is localized to activated cell surfaces expressing anionic phospholipids such as phosphatidylserine, and is mediated by Ca2+ bridging between the anionic phospholipids and g-carboxyglutamic acid residues of the clotting factors. This is the basis for using calcium chelators such as ethylenediamine tetraacetic acid (EDTA) or citrate to prevent blood from clotting in a test tube.
Antithrombin (AT) is an endogenous anticoagulant and a member of the serine protease inhibitor (serpin) family; it inactivates the serine proteases IIa, IXa, Xa, XIa, and XIIa. The endogenous anticoagulants protein C and protein S attenuate the blood clotting cascade by proteolysis of the two cofactors Va and VIIIa. From an evolutionary standpoint, it is of interest that factors V and VIII have an identical overall domain structure and considerable homology, consistent with a common ancestor gene; likewise the serine proteases are descendents of a trypsin-like common ancestor. Thus, the TF-VIIa initiating complex, serine proteases, and cofactors each have their own lineage-specific attenuation mechanism. Defects iatural anticoagulants result in an increased risk of venous thrombosis. The most common defect in the natural anticoagulant system is a mutation in factor V (factor V Leiden), which results in resistance to inactivation by the protein C, protein S mechanism.
Fibrinolysis refers to the process of fibrin digestion by the fibrin-specific protease, plasmin. The fibrinolytic system is similar to the coagulation system in that the precursor form of the serine protease plasmin circulates in an inactive form as plasminogen. In response to injury, endothelial cells synthesize and release tissue plasminogen activator (t-PA), which converts plasminogen to plasmin. Plasmin remodels the thrombus and limits its extension by proteolytic digestion of fibrin.
Both plasminogen and plasmin have specialized protein domains (kringles) that bind to exposed lysines on the fibrin clot and impart clot specificity to the fibrinolytic process. It should be noted that this clot specificity is only observed at physiologic levels of t-PA. At the pharmacologic levels of t-PA used in thrombolytic therapy, clot specificity is lost and a systemic lytic state is created, with attendant increase in bleeding risk. As in the coagulation cascade, there are negative regulators of fibrinolysis: endothelial cells synthesize and release plasminogen activator inhibitor (PAI), which inhibits t-PA; in addition a2 antiplasmin circulates in the blood at high concentrations and under physiologic conditions will rapidly inactivate any plasmin that is not clot-bound. However, this regulatory system is overwhelmed by therapeutic doses of plasminogen activators.
If the coagulation and fibrinolytic systems are pathologically activated, the hemostatic system may careen out of control, leading to generalized intravascular clotting and bleeding. This process is called disseminated intravascular coagulation (DIC) and may follow massive tissue injury, advanced cancers, obstetric emergencies such as abruptio placentae or retained products of conception, or bacterial sepsis. The treatment of DIC is to control the underlying disease process; if this is not possible, DIC is often fatal.
Regulation of the fibrinolytic system is useful in therapeutics. Increased fibrinolysis is effective therapy for thrombotic disease. Tissue plasminogen activator, urokinase, and streptokinase all activate the fibrinolytic system. Conversely, decreased fibrinolysis protects clots from lysis and reduces the bleeding of hemostatic failure. Aminocaproic acid is a clinically useful inhibitor of fibrinolysis. Heparin and the oral anticoagulant drugs do not affect the fibrinolytic mechanism.
I. BASIC PHARMACOLOGY OF THE ANTICOAGULANT DRUGS
INTRODUCTION
The ideal anticoagulant drug would prevent pathologic thrombosis and limit reperfusion injury, yet allow a normal response to vascular injury and limit bleeding. Theoretically this could be accomplished by preservation of the TF-VIIa initiation phase of the clotting mechanism with attenuation of the secondary intrinsic pathway propagation phase of clot development. At this time such a drug does not exist; all anticoagulants and fibrinolytic drugs have an increased bleeding risk as their principle toxicity.
The indirect thrombin inhibitors are so-named because their antithrombotic effect is exerted by their interaction with a separate protein, antithrombin. Unfractionated heparin (UFH), low-molecular-weight heparin (LMWH), and the synthetic pentasaccharide fondaparinux bind to antithrombin and enhance its inactivation of factor Xa. Unfractionated heparin and to a lesser extent LMWH also enhance antithrombin’s inactivation of thrombin.
HEPARIN
Chemistry & Mechanism of Action
Heparin is a heterogeneous mixture of sulfated mucopolysaccharides. It binds to endothelial cell surfaces and a variety of plasma proteins. Its biologic activity is dependent upon the endogenous anticoagulant antithrombin. Antithrombin inhibits clotting factor proteases, especially thrombin (IIa), IXa, and Xa, by forming equimolar stable complexes with them. In the absence of heparin, these reactions are slow; in the presence of heparin, they are accelerated 1000-fold. Only about a third of the molecules in commercial heparin preparations have an accelerating effect because the remainder lack the unique pentasaccharide sequence needed for high-affinity binding to antithrombin. The active heparin molecules bind tightly to antithrombin and cause a conformational change in this inhibitor. The conformational change of antithrombin exposes its active site for more rapid interaction with the proteases (the activated clotting factors). Heparin functions as a cofactor for the antithrombin-protease reaction without being consumed. Once the antithrombin-protease complex is formed, heparin is released intact for renewed binding to more antithrombin.
The antithrombin binding region of commercial unfractionated heparin consists of repeating sulfated disaccharide units composed of D-glucosamine-L-iduronic acid and D-glucosamine-D-glucuronic acid. High-molecular-weight fractions of heparin with high affinity for antithrombin markedly inhibit blood coagulation by inhibiting all three factors, especially thrombin and factor Xa. Unfractionated heparin has a molecular weight range of 5000-
Because commercial heparin consists of a family of molecules of different molecular weights, the correlation between the concentration of a given heparin preparation and its effect on coagulation often is poor. Therefore, UFH is standardized by bioassay. Heparin sodium USP must contain at least 120 USP units per milligram. Heparin is generally used as the sodium salt, but calcium heparin is equally effective. Lithium heparin is used in vitro as an anticoagulant for blood samples. Commercial heparin is extracted from porcine intestinal mucosa and bovine lung. Enoxaparin is obtained from the same sources as regular heparin, but doses are specified in milligrams. Dalteparin, tinzaparin and danaparoid (an LMW heparanoid containing heparan sulfate, dermatan sulfate, and chondroitin sulfate), on the other hand, are specified in anti-factor Xa units.
Close monitoring of the activated partial thromboplastin time (aPTT) is necessary in patients receiving UFH. Levels of UFH may also be determined by protamine titration (therapeutic levels 0.2-0.4 unit/mL) or anti-Xa units (therapeutic levels 0.3-0.7 unit/mL). Weight-based dosing of the LMW heparins results in predictable pharmacokinetics and plasma levels in patients with normal renal function. Therefore, LMW heparin levels are not generally measured except in the setting of renal insufficiency, obesity, and pregnancy. LMW heparin levels can be determined by anti-Xa units. Peak therapeutic levels should be 0.5-1 unit/mL for twice-daily dosing, determined 4 hours after administration, and approximately 1.5 units/mL for once-daily dosing.
Toxicity
A. BLEEDING
The major adverse effect of heparin is bleeding. This risk can be decreased by scrupulous patient selection, careful control of dosage, and close monitoring. Elderly women and patients with renal failure are more prone to hemorrhage. Heparin is of animal origin and should be used cautiously in patients with allergy. Increased loss of hair and reversible alopecia have been reported. Long-term heparin therapy is associated with osteoporosis and spontaneous fractures. Heparin accelerates the clearing of postprandial lipemia by causing the release of lipoprotein lipase from tissues, and long-term use is associated with mineralocorticoid deficiency.
B. HEPARIN-INDUCED THROMBOCYTOPENIA
Heparin-induced thrombocytopenia (HIT) is a systemic hypercoagulable state that occurs in 1-4% of individuals treated with UFH for a minimum of 7 days. Surgical patients are at greatest risk. The reported incidence of HIT is lower in pediatric populations outside the critical care setting and is relatively rare in pregnant women. The risk of HIT may be higher in individuals treated with UFH of bovine origin compared with porcine heparin and is lower in those treated exclusively with LMWH.
Morbidity and mortality in HIT are related to thrombotic events. Venous thrombosis occurs most commonly, but occlusion of peripheral or central arteries is not infrequent. If an indwelling catheter is present, the risk of thrombosis is increased in that extremity. Skiecrosis has been described, particularly in individuals treated with warfarin in the absence of a direct thrombin inhibitor, presumably due to acute depletion of the vitamin K-dependent anticoagulant protein C occurring in the presence of high levels of procoagulant proteins and an active hypercoagulable state.
The following points should be considered in all patients receiving heparin: Platelet counts should be performed frequently; thrombocytopenia appearing in a time frame consistent with an immune response to heparin should be considered suspicious for HIT; and any new thrombus occuring in a patient receiving heparin therapy should raise suspicion of HIT. Patients who develop HIT are treated by discontinuance of heparin and administration of a direct thrombin inhibitor or fondaparinux (see below).
Contraindications
Heparin is contraindicated in patients with HIT, hypersensitivity to the drug, active bleeding, hemophilia, significant thrombocytopenia, purpura, severe hypertension, intracranial hemorrhage, infective endocarditis, active tuberculosis, ulcerative lesions of the gastrointestinal tract, threatened abortion, visceral carcinoma, or advanced hepatic or renal disease. Heparin should be avoided in patients who have recently had surgery of the brain, spinal cord, or eye, and in patients who are undergoing lumbar puncture or regional anesthetic block. Despite the apparent lack of placental transfer, heparin should be used in pregnant women only when clearly indicated.
The indications for the use of heparin are described in the section on clinical pharmacology. A plasma concentration of heparin of 0.2-0.4 unit/mL (by protamine titration) or 0.3-0.7 unit/mL (anti-Xa units) usually prevents pulmonary emboli in patients with established venous thrombosis. This concentration of heparin will prolong the aPTT to 2-2.5 times that of the control value. This degree of anticoagulant effect should be maintained throughout the course of continuous intravenous heparin therapy. When intermittent heparin administration is used, the aPTT should be measured 6 hours after the administered dose to maintain prolongation of the aPTT to 2-2.5 times that of the control value.
Continuous intravenous administration of heparin is accomplished via an infusion pump. After an initial bolus injection of 80-100 units/kg, a continuous infusion of about 15-22 units/kg/h is required to maintain the aPTT at 2-2.5 times control. Patients with acute pulmonary emboli often require larger doses during the first few days because of binding to a variety of acute phase proteins, such as factor VIII and von Willebrand factor, and increased heparin clearance. Low-dose prophylaxis is achieved with subcutaneous administration of heparin, 5000 units every 8-12 hours. Because of the danger of hematoma formation at the injection site, heparin must never be administered intramuscularly.
Prophylactic enoxaparin is given subcutaneously in a dosage of 30 mg twice daily or 40 mg once daily. Full-dose enoxaparin therapy is 1 mg/kg subcutaneously every 12 hours. This corresponds to a therapeutic anti-factor Xa level of 0.5-1 unit/mL. Selected patients may be treated with enoxaparin 1.5 mg/kg once a day, with a target anti-Xa level of 1.5 units/mL. The prophylactic dose of dalteparin is 5000 units subcutaneously once a day; therapeutic dosing is 200 units/kg once a day for venous disease or 120 units/kg every 12 hours for acute coronary syndrome. Low-molecular-weight heparins should be used with caution in patients with renal insufficiency or body weight greater than
The synthetic pentasaccharide molecule fondaparinux avidly binds antithrombin with high specific activity, resulting in efficient inactivation of factor Xa. Fondaparinux has a long half-life of 15 hours, allowing for once-daily dosing by subcutaneous administration. Fondaparinux is effective in the prevention and treatment of venous thromboembolism, and appears to not cross-react with pathologic HIT antibodies in most individuals. The use of fondaparinux as an alternative anticoagulant in HIT is currently being tested in clinical trials. Pharmaceutical companies have put much effort into developing an orally bioavailable anti-Xa inhibitor. The first of these have recently completed phase I clinical trials with promising results and are currently being evaluated for efficacy in prophylaxis and treatment of venous thromboembolism.
Excessive anticoagulant action of heparin is treated by discontinuance of the drug. If bleeding occurs, administration of a specific antagonist such as protamine sulfate is indicated. Protamine is a highly basic peptide that combines with heparin as an ion pair to form a stable complex devoid of anticoagulant activity. For every 100 units of heparin remaining in the patient, 1 mg of protamine sulfate is given intravenously; the rate of infusion should not exceed 50 mg in any 10-minute period. Excess protamine must be avoided; it also has an anticoagulant effect. Neutralization of LMW heparin by protamine is incomplete. Limited experience suggests that 1 mg of protamine sulfate may be used to partially neutralize 1 mg of enoxaparin. Protamine will not reverse the activity of fondaparinux. Excess danaparoid can be removed by plasmapheresis.
The direct thrombin inhibitors (DTIs) exert their anticoagulant effect by directly binding to the active site of thrombin, thereby inhibiting thrombin’s downstream effects. This is in contrast to indirect thrombin inhibitors such as heparin and LMWH (see above), which act through antithrombin. Hirudin and bivalirudin are bivalent DTIs in that they bind at both the catalytic or active site of thrombin as well as at a substrate recognition site. Argatroban and melagatran are small molecules that bind only at the thrombin active site.
Leeches have been used for bloodletting since the age of Hippocrates. More recently, surgeons have used medicinal leeches (Hirudo medicinalis) to prevent thrombosis in the fine vessels of reattached digits. Hirudin is a specific, irreversible thrombin inhibitor from leech saliva that is now available in recombinant form as lepirudin. Its action is independent of antithrombin, which means it can reach and inactivate fibrin-bound thrombin in thrombi. Lepirudin has little effect on platelets or the bleeding time. Like heparin, it must be administered parenterally and is monitored by the aPTT. Lepirudin is approved by the Food and Drug Administration for use in patients with thrombosis related to heparin-induced thrombocytopenia. Lepirudin is excreted by the kidney and should be used with great caution in patients with renal insufficiency as no antidote exists. Up to 40% of patients who receive long-term infusions develop an antibody directed against the thrombin-lepirudin complex. These antigen-antibody complexes are not cleared by the kidney and may result in an enhanced anticoagulant effect. Some patients re-exposed to the drug have developed life-threatening anaphylactic reactions.
Bivalirudin, another bivalent inhibitor of thrombin, is administered intravenously, with a rapid onset and offset of action. The drug has a short half-life with clearance that is 20% renal and the remainder metabolic. Bivalirudin also inhibits platelet activation and has been FDA-approved for use in percutaneous coronary angioplasty.
Argatroban is a small molecule thrombin inhibitor that is FDA-approved for use in patients with HIT with or without thrombosis and coronary angioplasty in patients with HIT. It, too, has a short half-life, is given by continuous intravenous infusion, and is monitored by aPTT. Its clearance is not affected by renal disease but is dependent on liver function; dose reduction is required in patients with liver disease. Patients on argatroban will demonstrate elevated international normalized ratios (INRs), rendering the transition to warfarin difficult (ie, the INR will reflect contributions from both warfarin and argatroban). (INR is discussed in detail in the discussion of warfarin administration.) A nomogram is supplied by the manufacturer to assist in this transition. No properly designed head-to-head trials have been performed to determine whether argatroban or lepirudin is superior in the treatment of HIT. However in practice, the choice of which DTI to use in a patient with HIT is usually dictated by the condition of the clearing organ. If the patient has severe renal insufficiency, then argatroban would be preferred. If there is severe hepatic insufficiency, then lepirudin would be a better choice.
Ximelagatran is an oral prodrug that is metabolized to the DTI melagatran. Potential advantages of ximelagatran include predictable pharmacokinetics and bioavailability. This allows for fixed dosing and predictable anticoagulant response; no need for routine coagulation monitoring; lack of interaction with P450-interacting drugs; and rapid onset and offset of action, which allow for immediate anticoagulation and thus no need for overlap with additional anticoagulant drugs. While clinical trials found that ximelagatran was as effective as other anticoagulants in venous thromboembolism and atrial fibrillation, hepatic toxicity was observed in 5-10% of individuals treated for more than one month. Thus while there is much enthusiasm for a nontoxic oral anticoagulant that might replace warfarin and not require routine monitoring, no such drug is currently FDA-approved.
WARFARIN & THE COUMARIN ANTICOAGULANTS
The clinical use of the coumarin anticoagulants began with the discovery of an anticoagulant substance formed in spoiled sweet clover silage which caused hemorrhagic disease in cattle. At the behest of local farmers, a chemist at the University of Wisconsin identified the toxic agent as bishydroxycoumarin. A synthesized derivative, dicumarol and its congeners, most notably warfarin (Wisconsin Alumni Research Foundation, with “arin” from coumarin added; were initially used as rodenticides. In the 1950s warfarin (under the brand name Coumadin) was introduced as an antithrombotic agent in humans. Warfarin is one of the most commonly prescribed drugs, used by approximately 1.5 million individuals, and several studies have indicated that the drug is significantly underused in clinical situations where it has proven benefit.
Warfarin is generally administered as the sodium salt and has 100% bioavailability. Over 99% of racemic warfarin is bound to plasma albumin, which may contribute to its small volume of distribution (the albumin space), its long half-life in plasma (36 hours), and the lack of urinary excretion of unchanged drug. Warfarin used clinically is a racemic mixture composed of equal amounts of two enantiomorphs. The levorotatory S-warfarin is four times more potent than the dextrorotatory R-warfarin. This observation is useful in understanding the stereoselective nature of several drug interactions involving warfarin.
Coumarin anticoagulants block the g-carboxylation of several glutamate residues in prothrombin and factors VII, IX, and X as well as the endogenous anticoagulant proteins C and S. The blockade results in incomplete coagulation factor molecules that are biologically inactive. The protein carboxylation reaction is coupled to the oxidation of vitamin K. The vitamin must then be reduced to reactivate it. Warfarin prevents reductive metabolism of the inactive vitamin K epoxide back to its active hydroquinone form. Mutational change of the responsible enzyme, vitamin K epoxide reductase, can give rise to genetic resistance to warfarin in humans and especially in rats.
There is an 8- to 12-hour delay in the action of warfarin. Its anticoagulant effect results from a balance between partially inhibited synthesis and unaltered degradation of the four vitamin K-dependent clotting factors. The resulting inhibition of coagulation is dependent on their degradation half-lives in the circulation. These half-lives are 6, 24, 40, and 60 hours for factors VII, IX, X, and II, respectively. Larger initial doses of warfarin¾up to about 0.75 mg/kg¾hasten the onset of the anticoagulant effect. Beyond this dosage, the speed of onset is independent of the dose size. The only effect of a larger loading dose is to prolong the time that the plasma concentration of drug remains above that required for suppression of clotting factor synthesis. The only difference among oral anticoagulants in producing and maintaining hypoprothrombinemia is the half-life of each drug.
Toxicity
Warfarin crosses the placenta readily and can cause a hemorrhagic disorder in the fetus. Furthermore, fetal proteins with g-carboxyglutamate residues found in bone and blood may be affected by warfarin; the drug can cause a serious birth defect characterized by abnormal bone formation. Thus, warfarin should never be administered during pregnancy. Cutaneous necrosis with reduced activity of protein C sometimes occurs during the first weeks of therapy. Rarely, the same process causes frank infarction of the breast, fatty tissues, intestine, and extremities. The pathologic lesion associated with the hemorrhagic infarction is venous thrombosis, suggesting that it is caused by warfarin-induced depression of protein C synthesis.
Treatment with warfarin should be initiated with standard doses of 5-10 mg rather than the large loading doses formerly used. The initial adjustment of the prothrombin time takes about 1 week, which usually results in a maintenance dose of 5-7 mg/d. The prothrombin time (PT) should be increased to a level representing a reduction of prothrombin activity to 25% of normal and maintained there for long-term therapy. When the activity is less than 20%, the warfarin dosage should be reduced or omitted until the activity rises above 20%.
The therapeutic range for oral anticoagulant therapy is defined in terms of an international normalized ratio (INR). The INR is the prothrombin time ratio (patient prothrombin time/mean of normal prothrombin time for lab)ISI, where the ISI exponent refers to the International Sensitivity Index, and is dependent on the specific reagents and instruments used for the determination. The ISI serves to relate measured prothrombin times to a World Health Organization reference standard thromboplastin; thus the prothrombin times performed on different properly calibrated instruments with a variety of thromboplastin reagents should give the same INR results for a given sample. For most reagent and instrument combinations in current use, the ISI is close to 1, making the INR roughly the ratio of the patient prothrombin time to the meaormal prothrombin time. The recommended INR for prophylaxis and treatment of thrombotic disease is 2-3. Patients with some types of artificial heart valves (eg, tilting disk) or other medical conditions increasing thrombotic risk have a recommended range of 2.5-3.5.
Occasionally patients exhibit warfarin resistance, defined as progression or recurrence of a thrombotic event while in therapeutic range. These individuals may have their INR target raised (which is accompanied by an increase in bleeding risk) or be changed to an alternative form of anticoagulation (eg, daily injections of LMWH). Warfarin resistance is most commonly seen in patients with advanced cancers, typically of gastrointestinal origin (Trousseau’s syndrome). A recent study has demonstrated the superiority of LMWH over warfarin in preventing recurrent venous thromboembolism in patients with cancer.
The oral anticoagulants often interact with other drugs and with disease states. These interactions can be broadly divided into pharmacokinetic and pharmacodynamic effects. Pharmacokinetic mechanisms for drug interaction with oral anticoagulants are mainly enzyme induction, enzyme inhibition, and reduced plasma protein binding. Pharmacodynamic mechanisms for interactions with warfarin are synergism (impaired hemostasis, reduced clotting factor synthesis, as in hepatic disease), competitive antagonism (vitamin K), and an altered physiologic control loop for vitamin K (hereditary resistance to oral anticoagulants).
The most serious interactions with warfarin are those that increase the anticoagulant effect and the risk of bleeding. The most dangerous of these interactions are the pharmacokinetic interactions with the pyrazolones phenylbutazone and sulfinpyrazone. These drugs not only augment the hypoprothrombinemia but also inhibit platelet function and may induce peptic ulcer disease. The mechanisms for their hypoprothrombinemic interaction are a stereoselective inhibition of oxidative metabolic transformation of S-warfarin (the more potent isomer) and displacement of albumin-bound warfarin, increasing the free fraction. For this and other reasons, neither phenylbutazone nor sulfinpyrazone is in common use in the USA. Metronidazole, fluconazole, and trimethoprim-sulfamethoxazole also stereoselectively inhibit the metabolic transformation of S-warfarin, whereas amiodarone, disulfiram, and cimetidine inhibit metabolism of both enantiomorphs of warfarin. Aspirin, hepatic disease, and hyperthyroidism augment warfarin pharmacodynamically¾aspirin by its effect on platelet function and the latter two by increasing the turnover rate of clotting factors. The third-generation cephalosporins eliminate the bacteria in the intestinal tract that produce vitamin K and, like warfarin, also directly inhibit vitamin K epoxide reductase.
Barbiturates and rifampin cause a marked decrease of the anticoagulant effect by induction of the hepatic enzymes that transform racemic warfarin. Cholestyramine binds warfarin in the intestine and reduces its absorption and bioavailability.
Pharmacodynamic reductions of anticoagulant effect occur with vitamin K (increased synthesis of clotting factors), the diuretics chlorthalidone and spironolactone (clotting factor concentration), hereditary resistance (mutation of vitamin K reactivation cycle molecules), and hypothyroidism (decreased turnover rate of clotting factors).
Drugs with no significant effect on anticoagulant therapy include ethanol, phenothiazines, benzodiazepines, acetaminophen, opioids, indomethacin, and most antibiotics.
Excessive anticoagulant effect and bleeding from warfarin can be reversed by stopping the drug and administering oral or parenteral vitamin K1 (phytonadione), fresh-frozen plasma, prothrombin complex concentrates such as Bebulin and Proplex T, and recombinant factor VIIa (rFVIIa). The disappearance of excessive effect is not correlated with plasma warfarin concentrations but rather with reestablishment of normal activity of the clotting factors. A modest excess of anticoagulant effect without bleeding may require no more than cessation of the drug. The warfarin effect can be rapidly reversed in the setting of severe bleeding with the administration of prothrombin complex or rFVIIa coupled with intravenous vitamin K. It is important to note that due to the long half life of warfarin, a single dose of vitamin K or rFVIIa may not be sufficient.
II. BASIC PHARMACOLOGY OF THE FIBRINOLYTIC DRUGS
Introduction
Fibrinolytic drugs rapidly lyse thrombi by catalyzing the formation of the serine protease plasmin from its precursor zymogen, plasminogen. These drugs create a generalized lytic state when administered intravenously. Thus, both protective hemostatic thrombi and target thromboemboli are broken down. The Box: Thrombolytic Drugs for Acute Myocardial Infarction, describes the use of these drugs in one major application.
Streptokinase is a protein (but not an enzyme in itself) synthesized by streptococci that combines with the proactivator plasminogen. This enzymatic complex catalyzes the conversion of inactive plasminogen to active plasmin. Urokinase is a human enzyme synthesized by the kidney that directly converts plasminogen to active plasmin. Plasmin itself cannot be used because naturally occurring inhibitors in plasma prevent its effects. However, the absence of inhibitors for urokinase and the streptokinase-proactivator complex permit their use clinically. Plasmin formed inside a thrombus by these activators is protected from plasma antiplasmins, which allows it to lyse the thrombus from within.
Anistreplase (anisoylated plasminogen streptokinase activator complex; APSAC) consists of a complex of purified human plasminogen and bacterial streptokinase that has been acylated to protect the enzyme’s active site. When administered, the acyl group spontaneously hydrolyzes, freeing the activated streptokinase-proactivator complex. This product (recently discontinued in the USA) allows for rapid intravenous injection, greater clot selectivity (ie, more activity on plasminogen associated with clots than on free plasminogen in the blood), and more thrombolytic activity.
Plasminogen can also be activated endogenously by tissue plasminogen activators (t-PAs). These activators preferentially activate plasminogen that is bound to fibrin, which (in theory) confines fibrinolysis to the formed thrombus and avoids systemic activation. Human t-PA is manufactured as alteplase by means of recombinant DNA technology.
Reteplase is another recombinant human t-PA from which several amino acid sequences have been deleted. Reteplase is less expensive to produce than t-PA. Because it lacks the major fibrin-binding domain, reteplase is less fibrin-specific than t-PA. Tenecteplase is a mutant form of t-PA that has a longer half-life, and it can be given as an intravenous bolus. Tenecteplase is slightly more fibrin-specific than t-PA.
THROMBOLYTIC DRUGS FOR ACUTE MYOCARDIAL INFARCTION
The paradigm shift in 1980 on the causation of acute myocardial infarction to acute coronary occlusion by a thrombus created the rationale for thrombolytic therapy of this common lethal disease. At that time¾and for the first time¾intravenous thrombolytic therapy for acute myocardial infarction in the European Cooperative Study Group trial was found to reduce mortality significantly. Later studies, with thousands of patients in each trial, provided enough statistical power for the 20% reduction in mortality to be considered statistically significant. Although the standard of care in areas with adequate facilities and experience in percutaneous coronary intervention (PCI) now favors catheterization and placement of a stent, thrombolytic therapy is still very important where PCI is not readily available.
The proper selection of patients for thrombolytic therapy is critical. The diagnosis of acute myocardial infarction is made clinically and is confirmed by electrocardiography. Patients with ST-segment elevation and bundle branch block on electrocardiography have the best outcomes. All trials to date show the greatest benefit for thrombolytic therapy when it is given early, within 6 hours after symptomatic onset of acute myocardial infarction.
Thrombolytic drugs reduce the mortality of acute myocardial infarction. The early and appropriate use of any thrombolytic drug probably transcends possible advantages of a particular drug. Adjunctive drugs such as aspirin, heparin, b blockers, and angiotensin-converting enzyme (ACE) inhibitors reduce mortality even further. The principles of management are outlined in part 7 of the American Heart Association Guidelines, 2000.
Indications & Dosage
Administration of fibrinolytic drugs by the intravenous route is indicated in cases of pulmonary embolism with hemodynamic instability, severe deep venous thrombosis such as the superior vena caval syndrome, and ascending thrombophlebitis of the iliofemoral vein with severe lower extremity edema. These drugs are also given intra-arterially, especially for peripheral vascular disease.
Thrombolytic therapy in the management of acute myocardial infarction requires careful patient selection, the use of a specific thrombolytic agent, and the benefit of adjuvant therapy. Streptokinase is administered by intravenous infusion of a loading dose of 250,000 units, followed by 100,000 units/h for 24-72 hours. Patients with antistreptococcal antibodies can develop fever, allergic reactions, and therapeutic resistance. Urokinase requires a loading dose of 300,000 units given over 10 minutes and a maintenance dose of 300,000 units/h for 12 hours. Alteplase (t-PA) is given by intravenous infusion of 60 mg over the first hour and then 40 mg at a rate of 20 mg/h. Reteplase is given as two intravenous bolus injections of 10 units each, separated by 30 minutes. Tenecteplase is given as a single intravenous bolus of 0.5 mg/kg. Anistreplase (where available) is given as a single intravenous injection of 30 units over 3-5 minutes. A single course of fibrinolytic drugs is expensive: hundreds of dollars for streptokinase and thousands for urokinase and t-PA.
Recombinant t-PA has also been approved for use in acute ischmic stroke within 3 hours of symptom onset. In patients without hemorrhagic infarct or other contraindications, this therapy has been demonstrated to provide better outcomes in several randomized clinical trials. The recommended dose is 0.9 mg/kg, not to exceed 90 mg, with 10% given as a bolus and the remainder during a 1 hour infusion. Streptokinase has been associated with increased bleeding risk in acute ischemic stroke when given at a dose of 1.5 million units, and its use is not recommended in this setting.
III. BASIC PHARMACOLOGY OF ANTIPLATELET AGENTS
Platelet function is regulated by three categories of substances. The first group consists of agents generated outside the platelet that interact with platelet membrane receptors, eg, catecholamines, collagen, thrombin, and prostacyclin. The second category contains agents generated within the platelet that interact with membrane receptors, eg, ADP, prostaglandin D2, prostaglandin E2, and serotonin. The third group comprises agents generated within the platelet that act within the platelet, eg, prostaglandin endoperoxides and thromboxane A2, the cyclic nucleotides cAMP and cGMP, and calcium ion. From this list of agents, several targets for platelet inhibitory drugs have been identified: inhibition of prostaglandin synthesis (aspirin), inhibition of ADP-induced platelet aggregation (clopidogrel, ticlopidine), and blockade of glycoprotein IIb/IIIa receptors on platelets (abciximab, tirofiban, and eptifibatide). Dipyridamole and cilostazol are additional antiplatelet drugs.
The prostaglandin thromboxane A2 is an arachidonate product that causes platelets to change shape, release their granules, and aggregate. Drugs that antagonize this pathway interfere with platelet aggregation in vitro and prolong the bleeding time in vivo. Aspirin is the prototype of this class of drugs.
Aspirin inhibits the synthesis of thromboxane A2 by irreversible acetylation of the enzyme cyclooxygenase. Other salicylates and nonsteroidal anti-inflammatory drugs also inhibit cyclooxygenase but have a shorter duration of inhibitory action because they cannot acetylate cyclooxygenase; that is, their action is reversible.
The FDA has approved the use of 325 mg/d for primary prophylaxis of myocardial infarction but urges caution in this use of aspirin by the general population except when prescribed as an adjunct to risk factor management by smoking cessation and lowering of blood cholesterol and blood pressure. Meta-analysis of many published trials of aspirin and other antiplatelet agents confirms the value of this intervention in the secondary prevention of vascular events among patients with a history of vascular events.
CLOPIDOGREL & TICLOPIDINE
Clopidogrel and ticlopidine reduce platelet aggregation by inhibiting the ADP pathway of platelets. These drugs are thienopyridine derivatives that achieve their antiplatelet effects by irreversibly blocking the ADP receptor on platelets. Unlike aspirin, these drugs have no effect on prostaglandin metabolism. Randomized clinical trials with both drugs report efficacy in the prevention of vascular events among patients with transient ischemic attacks, completed strokes, and unstable angina pectoris. Use of clopidogrel or ticlopidine to prevent thrombosis is now considered standard practice in patients undergoing placement of a coronary stent.
Adverse effects of ticlopidine include nausea, dyspepsia, and diarrhea in up to 20% of patients, hemorrhage in 5%, and, most seriously, leukopenia in 1%. The leukopenia is detected by regular monitoring of the white blood cell count during the first 3 months of treatment. Development of thrombotic thrombocytopenic purpura has also been associated with the ingestion of ticlopidine. The dosage of ticlopidine is 250 mg twice daily. It is particularly useful in patients who cannot tolerate aspirin. Doses of ticlopidine less than 500 mg/d may be efficacious with fewer adverse effects.
Clopidogrel has fewer adverse effects than ticlopidine and is rarely associated with neutropenia. Thrombotic thrombocytopenic purpura associated with clopidogrel has been reported. Because of its superior side effect profile and dosing requirements, clopidogrel is preferred over ticlopidine. The antithrombotic effects of clopidogrel are dose-dependent; within 5 hours after an oral loading dose of 300 mg, 80% of platelet activity will be inhibited. The maintenance dose of clopidogrel is 75 mg/d, which achieves maximum platelet inhibition. The duration of the antiplatelet effect is 7-10 days.
Aspirin & Clopidogrel Resistance
The reported incidence of resistance to these drugs varies greatly, from less than 5% to 75%. In part this tremendous variation in incidence reflects the definition of resistance (recurrent thrombosis while on antiplatelet therapy vs in vitro testing), methods by which drug response is measured, and patient compliance. Several methods for testing aspirin and clopidogrel resistance in vitro are now FDA-approved; however, their utility outside of clinical trials remains controversial.
BLOCKADE OF PLATELET GLYCOPROTEIN IIB/IIIA RECEPTORS
The glycoprotein IIb/IIIa inhibitors are used in patients with acute coronary syndromes. These drugs target the platelet IIb/IIIa receptor complex. The IIb/IIIa complex functions as a receptor mainly for fibrinogen and vitronectin but also for fibronectin and von Willebrand factor. Activation of this receptor complex is the “final common pathway” for platelet aggregation. There are approximately 50,000 copies of this complex on the surface of each platelet. Persons lacking this receptor have a bleeding disorder called Glanzmann’s thrombasthenia.
Abciximab, a chimeric monoclonal antibody directed against the IIb/IIIa complex including the vibronectin receptor, was the first agent approved in this class of drugs. It has been approved for use in percutaneous coronary intervention and in acute coronary syndromes. Eptifibatide is an analog of the sequence at the extreme carboxyl terminal of the delta chain of fibrinogen, which mediates the binding of fibrinogen to the receptor. Tirofiban is a smaller molecule with similar properties. Eptifibatide and tirofiban inhibit ligand binding to the IIb/IIIa receptor by their occupancy of the receptor but do not block the vibronectin receptor.
The three agents described above are administered parenterally. Oral formulations of IIb/IIIa antagonists have been developed and are in various stages of development.
ADDITIONAL ANTIPLATELET-DIRECTED DRUGS
Dipyridamole is a vasodilator that inhibits platelet function by inhibiting adenosine uptake and cyclic GMP phosphodiesterase activity. Dipyridamole by itself has little or no beneficial effect. Therefore, therapeutic use of this agent is primarily in combination with aspirin to prevent cerebrovascular ischemia. It may also be used in combination with warfarin for primary prophylaxis of thromboemboli in patients with prosthetic heart valves. A combination of dipyridamole complexed with 25 mg of aspirin is now available for secondary prophylaxis of cerebrovascular disease.
Cilostazol is a newer phosphodiesterase inhibitor that promotes vasodilation and inhibition of platelet aggregation. Cilostazol is used primarily to treat intermittent claudication.
IV. CLINICAL PHARMACOLOGY OF DRUGS USED TO PREVENT CLOTTING
A. INHERITED DISORDERS
The inherited disorders characterized by a tendency to form thrombi (thrombophilia) derive from either quantitative or qualitative abnormalities of the natural anticoagulant system. Deficiencies (loss of function mutations) in the natural anticoagulants antithrombin, protein C, and protein S account for approximately 15% of selected patients with juvenile or recurrent thrombosis and 5-10% of unselected cases of acute venous thrombosis. Additional causes of thrombophilia include gain of function mutations such as the factor V Leiden mutation and the prothrombin 20210 mutation, elevated clotting factor and cofactor levels, and hyperhomocysteinemia that together account for the greater number of hypercoagulable patients. Although the loss of function mutations are less common, they are associated with the greatest thrombosis risk. Some patients have multiple inherited risk factors or combinations of inherited and acquired risk factors as discussed below. These individuals are at higher risk for recurrent thrombotic events and are often considered candidates for lifelong therapy.
B. ACQUIRED DISEASE
The increased risk of thromboembolism associated with atrial fibrillation and with the placement of mechanical heart valves has long been recognized. Similarly, prolonged bed rest, high-risk surgical procedures, and the presence of cancer are clearly associated with an increased incidence of deep venous thrombosis and embolism. Antiphospholipic antibody syndrome is another important acquired risk factor. Drugs may function as synergistic risk factors in concert with inherited risk factors. For example, women who have the factor V Leiden mutation and take oral contraceptives have a synergistic increase in risk.
A. PREVENTION
Primary prevention of venous thrombosis reduces the incidence of and mortality rate from pulmonary emboli. Heparin and warfarin may be used to prevent venous thrombosis. Subcutaneous administration of low-dose unfractionated heparin, low-molecular-weight heparin, or fondaparinux provides effective prophylaxis. Warfarin is also effective but requires laboratory monitoring of the prothrombin time.
B. TREATMENT OF ESTABLISHED DISEASE
Treatment for established venous thrombosis is initiated with unfractionated or low-molecular-weight heparin for the first 5-7 days, with an overlap with warfarin. Once therapeutic effects of warfarin have been established, therapy with warfarin is continued for a minimum of 3-6 months. Patients with recurrent disease or identifiable, nonreversible risk factors may be treated indefinitely. Small thrombi confined to the calf veins may be managed without anticoagulants if there is documentation over time that the thrombus is not extending.
Warfarin readily crosses the placenta. It can cause hemorrhage at any time during pregnancy as well as developmental defects when administered during the first trimester. Therefore, venous thromboembolic disease in pregnant women is generally treated with heparin, best administered by subcutaneous injection.
Activation of platelets is considered an essential process for arterial thrombosis. Thus, treatment with platelet-inhibiting drugs such as aspirin and clopidogrel or ticlopidine is indicated in patients with transient ischemic attacks and strokes or unstable angina and acute myocardial infarction. In angina and infarction, these drugs are often used in conjunction with b blockers, calcium channel blockers, and fibrinolytic drugs.
V. DRUGS USED IN BLEEDING DISORDERS
Vitamin K confers biologic activity upon prothrombin and factors VII, IX, and X by participating in their postribosomal modification. Vitamin K is a fat-soluble substance found primarily in leafy green vegetables. The dietary requirement is low, because the vitamin is additionally synthesized by bacteria that colonize the human intestine. Two natural forms exist: vitamins K1 and K2. Vitamin K1 (phytonadione); is found in food. Vitamin K2 (menaquinone) is found in human tissues and is synthesized by intestinal bacteria.
Vitamins K1 and K2 require bile salts for absorption from the intestinal tract. Vitamin K1 is available clinically in oral and parenteral forms. Onset of effect is delayed for 6 hours but the effect is complete by 24 hours when treating depression of prothrombin activity by excess warfarin or vitamin K deficiency. Intravenous administration of vitamin K1 should be slow, because rapid infusion can produce dyspnea, chest and back pain, and even death. Vitamin K repletion is best achieved with intravenous or oral administration, because its bioavailability after subcutaneous administration is erratic. Vitamin K1 is currently administered to all newborns to prevent the hemorrhagic disease of vitamin K deficiency, which is especially common in premature infants. The water-soluble salt of vitamin K3 (menadione) should never be used in therapeutics. It is particularly ineffective in the treatment of warfarin overdosage. Vitamin K deficiency frequently occurs in hospitalized patients in intensive care units because of poor diet, parenteral nutrition, recent surgery, multiple antibiotic therapy, and uremia. Severe hepatic failure results in diminished protein synthesis and a hemorrhagic diathesis that is unresponsive to vitamin K.
Deficiencies in plasma coagulation factors can cause bleeding. Spontaneous bleeding occurs when factor activity is less than 5-10% of normal. Factor VIII deficiency (classic hemophilia, or hemophilia A) and factor IX deficiency (Christmas disease, or hemophilia B) account for most of the heritable coagulation defects. Concentrated plasma fractions are available for the treatment of these deficiencies. Administration of plasma-derived, heat- or detergent-treated factor concentrates and recombinant factor concentrates are the standard treatments for bleeding associated with hemophilia. Lyophilized factor VIII concentrates are prepared from large pools of plasma. Transmission of viral diseases such as hepatitis B and C and HIV is reduced or eliminated by pasteurization and by extraction of plasma with solvents and detergents. However, this treatment does not remove other potential causes of transmissable diseases such as prions. For this reason, recombinant clotting factor preparations are recommended whenever possible for factor replacement. The best use of these therapeutic materials requires diagnostic specificity of the deficient factor and quantitation of its activity in plasma. Intermediate purity factor VIII concentrates (as opposed to recombinant or high purity concentrates) contain significant amounts of von Willebrand factor. Humate-P is a factor VIII concentrate that is approved by the FDA for the treatment of bleeding associated with von Willebrand disease.
An uncomplicated hemorrhage into a joint should be treated with sufficient factor VIII or factor IX replacement to maintain a level of at least 30-50% of the normal concentration for 24 hours. Soft tissue hematomas require a minimum of 100% activity for 7 days. Hematuria requires at least 10% activity for 3 days. Surgery and major trauma require a minimum of 100% activity for 10 days. The initial loading dose for factor VIII is 50 units/kg of body weight to achieve 100% activity of factor VIII from a baseline of £1%, assuming a normal hemoglobin. Each unit of factor VIII per kilogram of body weight raises its activity in plasma 2%. Replacement should be administered every 12 hours. Factor IX therapy requires twice the dose of factor VIII, but with an administration of about every 24 hours because of its longer half-life. Recombinant factor IX has only 80% recovery compared with plasma-derived factor IX products. Therefore, dosing with recombinant factor IX requires 120% of the dose used with the plasma-derived product.
Desmopressin acetate increases the factor VIII activity of patients with mild hemophilia A or von Willebrand disease. It can be used in preparation for minor surgery such as tooth extraction without any requirement for infusion of clotting factors if the patient has a documented adequate response. High-dose intranasal desmopressin is available and has been shown to be efficacious and well tolerated by patients.
Freeze-dried concentrates of plasma containing prothrombin, factors IX and X, and varied amounts of factor VII (Proplex, etc) are commercially available for treating deficiencies of these factors. Each unit of factor IX per kilogram of body weight raises its activity in plasma 1.5%. Heparin is often added to inhibit coagulation factors activated by the manufacturing process. However, addition of heparin does not eliminate all thromboembolic risk.
Some preparations of factor IX concentrate contain activated clotting factors, which has led to their use in treating patients with inhibitors or antibodies to factor VIII or factor IX. Two products are available expressly for this purpose: Autoplex (with factor VIII correctional activity) and FEIBA (Factor Eight Inhibitor Bypassing Activity). These products are not uniformly successful in arresting hemorrhage, and the factor IX inhibitor titers often rise after treatment with them. Acquired inhibitors of coagulation factors may also be treated with porcine factor VIII (for factor VIII inhibitors) and recombinant activated factor VII. Recombinant activated factor VII (NovoSeven) is being increasingly used to treat coagulopathy associated with liver disease and major blood loss in trauma and surgery. These recombinant and plasma-derived factor concentrates are very expensive, and the indications for them are very precise. Therefore, close consultation with a hematologist knowledgeable in this area is essential.
Cryoprecipitate is a plasma protein fraction obtainable from whole blood. It is used to treat deficiencies or qualitative abnormalities of fibrinogen, such as that which occurs with disseminated intravascular coagulation and liver disease. A single unit of cryoprecipitate contains 300 mg of fibrinogen.
Cryoprecipitate may also be used for patients with factor VIII deficiency and von Willebrand disease if desmopressin is not indicated and a pathogen-inactivated, recombinant, or plasma-derived product is not available. The concentration of factor VIII and von Willebrand factor in cryoprecipitate is not as great as that found in the concentrated plasma fractions. Moreover, cryoprecipitate is not treated in any manner to decrease the risk of viral exposure. For infusion, the frozen cryoprecipitate unit is thawed and dissolved in a small volume of sterile citrate-saline solution and pooled with other units. Rh-negative women with potential for childbearing should receive only Rh-negative cryoprecipitate because of possible contamination of the product with Rh-positive blood cells.
FIBRINOLYTIC INHIBITORS: AMINOCAPROIC ACID
Aminocaproic acid (EACA), which is chemically similar to the amino acid lysine, is a synthetic inhibitor of fibrinolysis. It competitively inhibits plasminogen activation. It is rapidly absorbed orally and is cleared from the body by the kidney. The usual oral dosage of EACA is
Clinical uses of aminocaproic acid are as adjunctive therapy in hemophilia, as therapy for bleeding from fibrinolytic therapy, and as prophylaxis for rebleeding from intracranial aneurysms. Treatment success has also been reported in patients with postsurgical gastrointestinal bleeding and postprostatectomy bleeding and bladder hemorrhage secondary to radiation- and drug-induced cystitis. Adverse effects of the drug include intravascular thrombosis from inhibition of plasminogen activator, hypotension, myopathy, abdominal discomfort, diarrhea, and nasal stuffiness. The drug should not be used in patients with disseminated intravascular coagulation or genitourinary bleeding of the upper tract, eg, kidney and ureters, because of the potential for excessive clotting.
SERINE PROTEASE INHIBITORS: APROTININ
Aprotinin is a serine protease inhibitor (“serpin”) that inhibits fibrinolysis by free plasmin and may have other antihemorrhagic effects as well. It also inhibits the plasmin-streptokinase complex in patients who have received that thrombolytic agent. Aprotinin will reduce bleeding¾by as much as 50%¾from many types of surgery, especially that involving extracorporeal circulation for open heart procedures and liver transplantation. It is currently approved for use in patients undergoing coronary artery bypass grafting who are at high risk of excessive blood loss. In earlier placebo-controlled trials, adverse effects of aprotinin were little different from those reported in patients in the placebo group. A more recent study indicated an increased risk of myocardial infarction, stroke, and renal damage in aprotinin-treated patients. In larger studies, a possible association with anaphylaxis has been reported in < 0.5% of cases. Therefore, a small test dose is recommended before the full therapeutic dose is given.
Hematopoiesis, the production from undifferentiated stem cells of circulating erythrocytes, platelets, and leukocytes, is a remarkable process that produces over 200 billioew blood cells per day in the normal person and even greater numbers of cells in people with conditions that cause loss or destruction of blood cells. The hematopoietic machinery resides primarily in the bone marrow in adults and requires a constant supply of three essential nutrients¾iron, vitamin B12, and folic acid¾as well as the presence of hematopoietic growth factors, proteins that regulate the proliferation and differentiation of hematopoietic cells. Inadequate supplies of either the essential nutrients or the growth factors result in deficiency of functional blood cells. Anemia, a deficiency in oxygen-carrying erythrocytes, is the most common and easily treated of these conditions, but thrombocytopenia and neutropenia are not rare and some forms are amenable to drug therapy. In this chapter, we first consider treatment of anemia due to deficiency of iron, vitamin B12, or folic acid and then turn to the medical use of hematopoietic growth factors to combat anemia, thrombocytopenia, and neutropenia, and to support stem cell transplantation.
Iron deficiency is the most common cause of chronic anemia. Like other forms of chronic anemia, iron deficiency anemia leads to pallor, fatigue, dizziness, exertional dyspnea, and other generalized symptoms of tissue hypoxia. The cardiovascular adaptations to chronic anemia¾tachycardia, increased cardiac output, vasodilation¾can worsen the condition of patients with underlying cardiovascular disease.
Iron forms the nucleus of the iron-porphyrin heme ring, which together with globin chains forms hemoglobin. Hemoglobin reversibly binds oxygen and provides the critical mechanism for oxygen delivery from the lungs to other tissues. In the absence of adequate iron, small erythrocytes with insufficient hemoglobin are formed, giving rise to microcytic hypochromic anemia.
Free inorganic iron is extremely toxic, but iron is required for essential proteins such as hemoglobin; therefore, evolution has provided an elaborate system for regulating iron absorption, transport, and storage. The system uses specialized transport and storage proteins whose concentrations are controlled by the body’s demand for hemoglobin synthesis and adequate iron stores. Nearly all of the iron used to support hematopoiesis is reclaimed from catalysis of the hemoglobin in senescent or damaged erythrocytes. Normally, only a small amount of iron is lost from the body each day, so dietary requirements are small and easily fulfilled by the iron available in a wide variety of foods. However, in special populations with either increased iron requirements (eg, growing children, pregnant women) or increased losses of iron (eg, menstruating women), iron requirements can exceed normal dietary supplies and iron deficiency can develop.
A. ABSORPTION
The average diet in the USA contains 10-15 mg of elemental iron daily. A normal individual absorbs 5-10% of this iron, or about 0.5-1 mg daily. Iron is normally absorbed in the duodenum and proximal jejunum, although the more distal small intestine can absorb iron if necessary. Iron absorption increases in response to low iron stores or increased iron requirements. Total iron absorption increases to 1-2 mg/d iormal menstruating women and may be as high as 3-4 mg/d in pregnant women.
Iron is available in a wide variety of foods but is especially abundant in meat. The iron in meat protein can be efficiently absorbed, because heme iron in meat hemoglobin and myoglobin can be absorbed intact without first having to be dissociated into elemental iron. Iron in other foods, especially vegetables and grains, is often tightly bound to organic compounds and is much less available for absorption. Nonheme iron in foods and iron in inorganic iron salts and complexes must be reduced to ferrous iron (Fe2+) before it can be absorbed by intestinal mucosal cells.
Iron crosses the luminal membrane of the intestinal mucosal cell by two mechanisms: active transport of ferrous iron and absorption of iron complexed with heme. The divalent metal transporter, DMT1, efficiently transports ferrous iron across the luminal membrane of the intestinal enterocyte. The rate of iron uptake is regulated by mucosal cell iron stores such that more iron is transported when stores are low. Together with iron split from absorbed heme, the newly absorbed iron can be actively transported into the blood across the basolateral membrane, probably by the transporter IREG1, also known as ferroportin1. Other proteins are involved in this process, and some of them are regulated to control iron absorption and storage. Excess iron can be stored in the mucosal cell as ferritin, a water-soluble complex consisting of a core of ferric hydroxide covered by a shell of a specialized storage protein called apoferritin. In general, when total body iron stores are high and iron requirements by the body are low, newly absorbed iron is diverted into ferritin in the intestinal mucosal cells. When iron stores are low or iron requirements are high, newly absorbed iron is immediately transported from the mucosal cells to the bone marrow to support hemoglobin production.
B. TRANSPORT
Iron is transported in the plasma bound to transferrin, a b-globulin that specifically binds two molecules of ferrous iron. The transferrin-iron complex enters maturing erythroid cells by a specific receptor mechanism. Transferrin receptors¾integral membrane glycoproteins present in large numbers on proliferating erythroid cells¾bind and internalize the transferrin-iron complex through the process of receptor-mediated endocytosis. In endosomes, the iron is released and funneled into hemoglobin synthesis, whereas the transferrin-transferrin receptor complex is recycled to the plasma membrane, where the transferrin dissociates and returns to the plasma. This process provides an efficient mechanism for supplying the iron required by developing red blood cells.
Increased erythropoiesis is associated with an increase in the number of transferrin receptors on developing erythroid cells. Iron store depletion and iron deficiency anemia are associated with an increased concentration of serum transferrin.
C. STORAGE
In addition to the storage of iron in intestinal mucosal cells, iron is also stored, primarily as ferritin, in macrophages in the liver, spleen, and bone, and in parenchymal liver cells. Apoferritin synthesis is regulated by the levels of free iron. When these levels are low, apoferritin synthesis is inhibited and the balance of iron binding shifts toward transferrin. When free iron levels are high, more apoferritin is produced to sequester more iron and protect organs from the toxic effects of excess free iron.
Ferritin is detectable in serum. Since the ferritin present in serum is in equilibrium with storage ferritin in reticuloendothelial tissues, the serum ferritin level can be used to estimate total body iron stores.
D. ELIMINATION
There is no mechanism for excretion of iron. Small amounts are lost in the feces by exfoliation of intestinal mucosal cells, and trace amounts are excreted in bile, urine, and sweat. These losses account for no more than 1 mg of iron per day. Because the body’s ability to excrete iron is so limited, regulation of iron balance must be achieved by changing intestinal absorption and storage of iron, in response to the body’s needs. As noted below, impaired regulation of iron absorption leads to serious pathology.
A. INDICATIONS FOR THE USE OF IRON
The only clinical indication for the use of iron preparations is the treatment or prevention of iron deficiency anemia. Iron deficiency is commonly seen in populations with increased iron requirements. These include infants, especially premature infants; children during rapid growth periods; pregnant and lactating women; and patients with chronic kidney disease who lose erythrocytes at a relatively high rate during hemodialysis and also form them at a high rate as a result of treatment with the erythrocyte growth factor erythropoietin (see below). Inadequate iron absorption can also cause iron deficiency. This is seen frequently after gastrectomy and in patients with severe small bowel disease that results in generalized malabsorption. Iron deficiency in these gastrointestinal conditions is due to inadequate iron absorption.
The most common cause of iron deficiency in adults is blood loss. Menstruating women lose about 30 mg of iron with each menstrual period; women with heavy menstrual bleeding may lose much more. Thus, many premenopausal women have low iron stores or even iron deficiency. In men and postmenopausal women, the most common site of blood loss is the gastrointestinal tract. Patients with unexplained iron deficiency anemia should be evaluated for occult gastrointestinal bleeding.
B. TREATMENT
Iron deficiency anemia is treated with oral or parenteral iron preparations. Oral iron corrects the anemia just as rapidly and completely as parenteral iron in most cases if iron absorption from the gastrointestinal tract is normal. An exception is the high requirement for iron of patients with advanced chronic kidney disease who are undergoing hemodialysis and treatment with erythropoietin; for these patients, parenteral iron administration is preferred.
1. Oral iron therapy¾ A wide variety of oral iron preparations are available. Because ferrous iron is most efficiently absorbed, only ferrous salts should be used. Ferrous sulfate, ferrous gluconate, and ferrous fumarate are all effective and inexpensive and are recommended for the treatment of most patients.
In an iron-deficient individual, about 50-100 mg of iron can be incorporated into hemoglobin daily, and about 25% of oral iron given as ferrous salt can be absorbed. Therefore, 200-400 mg of elemental iron should be given daily to correct iron deficiency most rapidly. Patients unable to tolerate such large doses of iron can be given lower daily doses of iron, which results in slower but still complete correction of iron deficiency. Treatment with oral iron should be continued for 3-6 months after correction of the cause of the iron loss. This corrects the anemia and replenishes iron stores.
Common adverse effects of oral iron therapy include nausea, epigastric discomfort, abdominal cramps, constipation, and diarrhea. These effects are usually dose-related and can often be overcome by lowering the daily dose of iron or by taking the tablets immediately after or with meals. Some patients have less severe gastrointestinal adverse effects with one iron salt than another and benefit from changing preparations. Patients taking oral iron develop black stools; this has no clinical significance in itself but may obscure the diagnosis of continued gastrointestinal blood loss.
2. Parenteral iron therapy¾ Parenteral therapy should be reserved for patients with documented iron deficiency who are unable to tolerate or absorb oral iron and for patients with extensive chronic blood loss who cannot be maintained with oral iron alone. This includes patients with various postgastrectomy conditions and previous small bowel resection, inflammatory bowel disease involving the proximal small bowel, malabsorption syndromes, and advanced chronic renal disease including hemodialysis and treatment with erythropoietin.
Iron dextran is a stable complex of ferric hydroxide and low-molecular-weight dextran containing 50 mg of elemental iron per milliliter of solution. It can be given by deep intramuscular injection or by intravenous infusion, although the intravenous route is used most commonly. Intravenous administration eliminates the local pain and tissue staining that often occur with the intramuscular route and allows delivery of the entire dose of iron necessary to correct the iron deficiency at one time. Adverse effects of intravenous iron dextran therapy include headache, light-headedness, fever, arthralgias, nausea and vomiting, back pain, flushing, urticaria, bronchospasm, and, rarely, anaphylaxis and death. Some of these effects represent a hypersensitivity reaction to the dextran component. Hypersensitivity reactions may be delayed for 48-72 hours after administration. Anaphylactic reactions to iron dextran, including fatal reactions, have been clearly documented. Owing to the risk of a hypersensitivity reaction, a small test dose of iron dextran should always be given before full intramuscular or intravenous doses are given. Patients with a strong history of allergy and patients who have previously received parenteral iron dextran are more likely to have hypersensitivity reactions after treatment with parenteral iron dextran.
Iron-sucrose complex and iron sodium gluconate complex are alternative preparations. These agents can be given only by the intravenous route. These preparations appear to be much less likely than iron dextran to cause hypersensitivity reactions.
For patients who are treated chronically with parenteral iron, it is important to periodically monitor iron storage levels to avoid the serious toxicity associated with iron overload. Unlike oral iron therapy, which is subject to the regulatory mechanism provided by the intestinal uptake system, parenteral administration, which bypasses this regulatory system, can deliver more iron than can be safely stored in intestinal cells and macrophages in the liver and tissues. Iron stores can be estimated on the basis of serum concentrations of ferritin and the transferrin saturation, which is the ratio of the total serum iron concentration to the total iron-binding capacity (TIBC).
Clinical Toxicity
A. ACUTE IRON TOXICITY
Acute iron toxicity is seen almost exclusively in young children who accidentally ingest iron tablets. Although adults are able to tolerate large doses of oral iron without serious consequences, as few as 10 tablets of any of the commonly available oral iron preparations can be lethal in young children. Adult patients taking oral iron preparations should be instructed to store tablets in child-proof containers out of the reach of children. Children who are poisoned with oral iron experience necrotizing gastroenteritis, with vomiting, abdominal pain, and bloody diarrhea followed by shock, lethargy, and dyspnea. Subsequently, improvement is ofteoted, but this may be followed by severe metabolic acidosis, coma, and death. Urgent treatment is necessary. Whole bowel irrigation should be performed to flush out unabsorbed pills. Deferoxamine, a potent iron-chelating compound, can be given systemically to bind iron that has already been absorbed and to promote its excretion in urine and feces. Activated charcoal, a highly effective adsorbent for most toxins, does not bind iron and thus is ineffective. Appropriate supportive therapy for gastrointestinal bleeding, metabolic acidosis, and shock must also be provided.
B. CHRONIC IRON TOXICITY
Chronic iron toxicity (iron overload), also known as hemochromatosis, results when excess iron is deposited in the heart, liver, pancreas, and other organs. It can lead to organ failure and death. It most commonly occurs in patients with inherited hemochromatosis, a disorder characterized by excessive iron absorption, and in patients who receive many red cell transfusions over a long period of time (eg, patients with thalassemia major).
Chronic iron overload in the absence of anemia is most efficiently treated by intermittent phlebotomy. One unit of blood can be removed every week or so until all of the excess iron is removed. Iron chelation therapy using parenteral deferoxamine is much less efficient as well as more complicated, expensive, and hazardous, but it can be the only option for iron overload that cannot be managed by phlebotomy, such as the iron overload experienced by patients with thalassemia major.
Recently, an oral iron chelator deferasirox has been approved for treatment of iron overload. Deferasirox appears to be as effective as deferoxamine at reducing liver iron concentrations and is much more convenient. However, it is not clear whether deferasirox is as effective as deferoxamine at protecting the heart from iron overload.
Vitamin B12 serves as a cofactor for several essential biochemical reactions in humans. Deficiency of vitamin B12 leads to anemia, gastrointestinal symptoms, and neurologic abnormalities. Although deficiency of vitamin B12 due to an inadequate supply in the diet is unusual, deficiency of B12 in adults¾especially older adults¾due to inadequate absorption of dietary vitamin B12 is a relatively common and easily treated disorder.
Chemistry
Vitamin B12 consists of a porphyrin-like ring with a central cobalt atom attached to a nucleotide. Various organic groups may be covalently bound to the cobalt atom, forming different cobalamins. Deoxyadenosylcobalamin and methylcobalamin are the active forms of the vitamin in humans. Cyanocobalamin and hydroxocobalamin (both available for therapeutic use) and other cobalamins found in food sources are converted to the active forms. The ultimate source of vitamin B12 is from microbial synthesis; the vitamin is not synthesized by animals or plants. The chief dietary source of vitamin B12 is microbially derived vitamin B12 in meat (especially liver), eggs, and dairy products. Vitamin B12 is sometimes called extrinsic factor to differentiate it from intrinsic factor, a proteiormally secreted by the stomach.
The average diet in the USA contains 5-30 mcg of vitamin B12 daily, 1-5 mcg of which is usually absorbed. The vitamin is avidly stored, primarily in the liver, with an average adult having a total vitamin B12 storage pool of 3000-5000 mcg. Only trace amounts of vitamin B12 are normally lost in urine and stool. Because the normal daily requirements of vitamin B12 are only about 2 mcg, it would take about 5 years for all of the stored vitamin B12 to be exhausted and for megaloblastic anemia to develop if B12 absorption stopped. Vitamin B12 in physiologic amounts is absorbed only after it complexes with intrinsic factor, a glycoprotein secreted by the parietal cells of the gastric mucosa. Intrinsic factor combines with the vitamin B12 that is liberated from dietary sources in the stomach and duodenum, and the intrinsic factor-vitamin B12 complex is subsequently absorbed in the distal ileum by a highly specific receptor-mediated transport system. Vitamin B12 deficiency in humans most often results from malabsorption of vitamin B12 due either to lack of intrinsic factor or to loss or malfunction of the specific absorptive mechanism in the distal ileum. Nutritional deficiency is rare but may be seen in strict vegetarians after many years without meat, eggs, or dairy products.
Once absorbed, vitamin B12 is transported to the various cells of the body bound to a plasma glycoprotein, transcobalamin II. Excess vitamin B12 is transported to the liver for storage.
Two essential enzymatic reactions in humans require vitamin B12. In one, methylcobalamin serves as an intermediate in the transfer of a methyl group from N5-methyltetrahydrofolate to homocysteine, forming methionine. Without vitamin B12, conversion of the major dietary and storage folate, N5-methyltetrahydrofolate, to tetrahydrofolate, the precursor of folate cofactors, cannot occur. As a result, a deficiency of folate cofactors necessary for several biochemical reactions involving the transfer of one-carbon groups develops. In particular, the depletion of tetrahydrofolate prevents synthesis of adequate supplies of the deoxythymidylate (dTMP) and purines required for DNA synthesis in rapidly dividing cells. The accumulation of folate as N5-methyltetrahydrofolate and the associated depletion of tetrahydrofolate cofactors in vitamin B12 deficiency have been referred to as the “methylfolate trap.” This is the biochemical step whereby vitamin B12 and folic acid metabolism are linked, and it explains why the megaloblastic anemia of vitamin B12 deficiency can be partially corrected by ingestion of relatively large amounts of folic acid. Folic acid can be reduced to dihydrofolate by the enzyme dihydrofolate reductase and thus serve as a source of the tetrahydrofolate required for synthesis of the purines and dTMP that are needed for DNA synthesis.
The other enzymatic reaction that requires vitamin B12 is isomerization of methylmalonyl-CoA to succinyl-CoA by the enzyme methylmalonyl-CoA mutase. In vitamin B12 deficiency, this conversion cannot take place, and the substrate, methylmalonyl-CoA, accumulates. In the past, it was thought that abnormal accumulation of methylmalonyl-CoA causes the neurologic manifestations of vitamin B12 deficiency. However, newer evidence instead implicates the disruption of the methionine synthesis pathway as the cause of neurologic problems. Whatever the biochemical explanation for neurologic damage, the important point is that administration of folic acid in the setting of vitamin B12 deficiency will not prevent neurologic manifestations even though it will largely correct the anemia caused by the vitamin B12 deficiency.
Vitamin B12 is used to treat or prevent deficiency. There is no evidence that vitamin B12 injections have any benefit in persons who do not have vitamin B12 deficiency. The most characteristic clinical manifestation of vitamin B12 deficiency is megaloblastic anemia. The typical clinical findings in megaloblastic anemia are macrocytic anemia, often with associated mild or moderate leukopenia or thrombocytopenia (or both), and a characteristic hypercellular bone marrow with an accumulation of megaloblastic erythroid and other precursor cells. The neurologic syndrome associated with vitamin B12 deficiency usually begins with paresthesias and weakness in peripheral nerves and progresses to spasticity, ataxia, and other central nervous system dysfunctions. Correction of vitamin B12 deficiency arrests the progression of neurologic disease, but it may not fully reverse neurologic symptoms that have been present for several months. Although most patients with neurologic abnormalities caused by vitamin B12 deficiency have megaloblastic anemia when first seen, occasional patients have few if any hematologic abnormalities.
Once a diagnosis of megaloblastic anemia is made, it must be determined whether vitamin B12 or folic acid deficiency is the cause. (Other causes of megaloblastic anemia are very rare.) This can usually be accomplished by measuring serum levels of the vitamins. The Schilling test, which measures absorption and urinary excretion of radioactively labeled vitamin B12, can be used to further define the mechanism of vitamin B12 malabsorption when this is found to be the cause of the megaloblastic anemia.
The most common causes of vitamin B12 deficiency are pernicious anemia, partial or total gastrectomy, and conditions that affect the distal ileum, such as malabsorption syndromes, inflammatory bowel disease, or small bowel resection.
Pernicious anemia results from defective secretion of intrinsic factor by the gastric mucosal cells. Patients with pernicious anemia have gastric atrophy and fail to secrete intrinsic factor (as well as hydrochloric acid). The Schilling test shows diminished absorption of radioactively labeled vitamin B12, which is corrected when intrinsic factor is administered with radioactive B12, since the vitamin can then be normally absorbed.
Vitamin B12 deficiency also occurs when the region of the distal ileum that absorbs the vitamin B12-intrinsic factor complex is damaged, as when the ileum is involved with inflammatory bowel disease or when the ileum is surgically resected. In these situations, radioactively labeled vitamin B12 is not absorbed in the Schilling test, even when intrinsic factor is added. Other rare causes of vitamin B12 deficiency include bacterial overgrowth of the small bowel, chronic pancreatitis, and thyroid disease. Rare cases of vitamin B12 deficiency in children have been found to be secondary to congenital deficiency of intrinsic factor and congenital selective vitamin B12 malabsorption due to defects of the receptor sites in the distal ileum.
Almost all cases of vitamin B12 deficiency are caused by malabsorption of the vitamin; therefore, parenteral injections of vitamin B12 are required for therapy. For patients with potentially reversible diseases, the underlying disease should be treated after initial treatment with parenteral vitamin B12. Most patients, however, do not have curable deficiency syndromes and require lifelong treatment with vitamin B12.
Vitamin B12 for parenteral injection is available as cyanocobalamin or hydroxocobalamin. Hydroxocobalamin is preferred because it is more highly protein-bound and therefore remains longer in the circulation. Initial therapy should consist of 100-1000 mcg of vitamin B12 intramuscularly daily or every other day for 1-2 weeks to replenish body stores. Maintenance therapy consists of 100-1000 mcg intramuscularly once a month for life. If neurologic abnormalities are present, maintenance therapy injections should be given every 1-2 weeks for 6 months before switching to monthly injections. Oral vitamin B12-intrinsic factor mixtures and liver extracts should not be used to treat vitamin B12 deficiency; however, oral doses of 1000 mcg of vitamin B12 daily are usually sufficient to treat patients with pernicious anemia who refuse or cannot tolerate the injections. After pernicious anemia is in remission following parenteral vitamin B12 therapy, the vitamin can be administered intranasally as a spray or gel.
Reduced forms of folic acid are required for essential biochemical reactions that provide precursors for the synthesis of amino acids, purines, and DNA. Folate deficiency is not uncommon, even though the deficiency is easily corrected by administration of folic acid. The consequences of folate deficiency go beyond the problem of anemia because folate deficiency is implicated as a cause of congenital malformations iewborns and may play a role in vascular disease
Chemistry
Folic acid (pteroylglutamic acid) is composed of a heterocycle (pteridine), p-aminobenzoic acid, and glutamic acid. Various numbers of glutamic acid moieties may be attached to the pteroyl portion of the molecule, resulting in monoglutamates, triglutamates, or polyglutamates. Folic acid can undergo reduction, catalyzed by the enzyme dihydrofolate reductase (“folate reductase”), to give dihydrofolic acid. Tetrahydrofolate can subsequently be transformed to folate cofactors possessing one-carbon units attached to the 5-nitrogen, to the 10-nitrogen, or to both positions. The folate cofactors are interconvertible by various enzymatic reactions and serve the important biochemical function of donating one-carbon units at various levels of oxidation. In most of these, tetrahydrofolate is regenerated and becomes available for reutilization.
The average diet in the USA contains 500-700 mcg of folates daily, 50-200 mcg of which is usually absorbed, depending on metabolic requirements. Pregnant women may absorb as much as 300-400 mcg of folic acid daily. Various forms of folic acid are present in a wide variety of plant and animal tissues; the richest sources are yeast, liver, kidney, and green vegetables. Normally, 5-20 mg of folates are stored in the liver and other tissues. Folates are excreted in the urine and stool and are also destroyed by catabolism, so serum levels fall within a few days when intake is diminished. Because body stores of folates are relatively low and daily requirements high, folic acid deficiency and megaloblastic anemia can develop within 1-6 months after the intake of folic acid stops, depending on the patient’s nutritional status and the rate of folate utilization.
Unaltered folic acid is readily and completely absorbed in the proximal jejunum. Dietary folates, however, consist primarily of polyglutamate forms of N5-methyltetrahydrofolate. Before absorption, all but one of the glutamyl residues of the polyglutamates must be hydrolyzed by the enzyme a-1-glutamyl transferase (“conjugase”) within the brush border of the intestinal mucosa. The monoglutamate N5-methyltetrahydrofolate is subsequently transported into the bloodstream by both active and passive transport and is then widely distributed throughout the body. Inside cells, N5-methyltetrahydrofolate is converted to tetrahydrofolate by the demethylation reaction that requires vitamin B12.
Tetrahydrofolate cofactors participate in one-carbon transfer reactions. As described earlier in the discussion of vitamin B12, one of these essential reactions produces the dTMP needed for DNA synthesis. In this reaction, the enzyme thymidylate synthase catalyzes the transfer of the one-carbon unit of N5, N10-methylenetetrahydrofolate to deoxyuridine monophosphate (dUMP) to form dTMP. Unlike all the other enzymatic reactions that use folate cofactors, in this reaction the cofactor is oxidized to dihydrofolate, and for each mole of dTMP produced, 1 mole of tetrahydrofolate is consumed. In rapidly proliferating tissues, considerable amounts of tetrahydrofolate are consumed in this reaction, and continued DNA synthesis requires continued regeneration of tetrahydrofolate by reduction of dihydrofolate, catalyzed by the enzyme dihydrofolate reductase. The tetrahydrofolate thus produced can then reform the cofactor N5,N10-methylenetetrahydrofolate by the action of serine transhydroxymethylase and thus allow for the continued synthesis of dTMP. The combined catalytic activities of dTMP synthase, dihydrofolate reductase, and serine transhydroxymethylase are often referred to as the dTMP synthesis cycle. Enzymes in the dTMP cycle are the targets of two anticancer drugs; methotrexate inhibits dihydrofolate reductase, and a metabolite of 5-fluorouracil inhibits thymidylate synthase.
Cofactors of tetrahydrofolate participate in several other essential reactions. N5-Methylenetetrahydrofolate is required for the vitamin B12-dependent reaction that generates methionine from homocysteine. In addition, tetrahydrofolate cofactors donate one-carbon units during the de novo synthesis of essential purines. In these reactions, tetrahydrofolate is regenerated and can reenter the tetrahydrofolate cofactor pool.
Folate deficiency results in a megaloblastic anemia that is microscopically indistinguishable from the anemia caused by vitamin B12 deficiency (see above). However, folate deficiency does not cause the characteristic neurologic syndrome seen in vitamin B12 deficiency. In patients with megaloblastic anemia, folate status is assessed with assays for serum folate or for red blood cell folate. Red blood cell folate levels are often of greater diagnostic value than serum levels, because serum folate levels tend to be labile and do not necessarily reflect tissue levels.
Folic acid deficiency, unlike vitamin B12 deficiency, is often caused by inadequate dietary intake of folates. Patients with alcohol dependence and patients with liver disease often develop folic acid deficiency because of poor diet and diminished hepatic storage of folates. Pregnant women and patients with hemolytic anemia have increased folate requirements and may become folic acid-deficient, especially if their diets are marginal. Evidence implicates maternal folic acid deficiency in the occurrence of fetal neural tube defects, eg, spina bifida. Patients with malabsorption syndromes also frequently develop folic acid deficiency. Patients who require renal dialysis develop folic acid deficiency because folates are removed from the plasma during the dialysis procedure.
Folic acid deficiency can be caused by drugs. Methotrexate and, to a lesser extent, trimethoprim and pyrimethamine, inhibit dihydrofolate reductase and may result in a deficiency of folate cofactors and ultimately in megaloblastic anemia. Long-term therapy with phenytoin can also cause folate deficiency, but only rarely causes megaloblastic anemia.
Parenteral administration of folic acid is rarely necessary, since oral folic acid is well absorbed even in patients with malabsorption syndromes. A dose of 1 mg folic acid orally daily is sufficient to reverse megaloblastic anemia, restore normal serum folate levels, and replenish body stores of folates in almost all patients. Therapy should be continued until the underlying cause of the deficiency is removed or corrected. Therapy may be required indefinitely for patients with malabsorption or dietary inadequacy. Folic acid supplementation to prevent folic acid deficiency should be considered in high-risk patients, including pregnant women, patients with alcohol dependence, hemolytic anemia, liver disease, or certain skin diseases, and patients on renal dialysis.
FOLIC ACID SUPPLEMENTATION: A PUBLIC HEALTH DILEMMA
Starting in January 1998, all products made from enriched grains in the USA were required to be supplemented with folic acid. This FDA ruling was issued to reduce the incidence of congenital neural tube defects. Epidemiologic studies show a strong correlation between maternal folic acid deficiency and the incidence of neural tube defects such as spina bifida and anencephaly. The FDA requirement for folic acid supplementation is a public health measure aimed at the significant number of women in the USA who do not receive prenatal care and are not aware of the importance of adequate folic acid ingestion for preventing birth defects in their babies.
There may be an added benefit for adults. N5-Methyltetrahydrofolate is required for the conversion of homocysteine to methionine. Impaired synthesis of N5-methyltetrahydrofolate results in elevated serum concentrations of homocysteine. Data from several sources suggest a positive correlation between elevated serum homocysteine and occlusive vascular diseases such as ischemic heart disease and stroke. Clinical data suggest that the folate supplementation program has improved the folate status and reduced the prevalence of hyperhomocysteinemia in a population of middle-aged and older adults who did not use vitamin supplements. It is possible, although the evidence thus far has beeegative, that the increased ingestion of folic acid will also reduce the risk of vascular disease in this population.
Although the potential benefits of supplemental folic acid during pregnancy are compelling, the decision to require folic acid in grains was¾and still is¾controversial. As described in the text, ingestion of folic acid can partially or totally correct the anemia caused by vitamin B12 deficiency. However, folic acid supplementation does not prevent the potentially irreversible neurologic damage caused by vitamin B12 deficiency. People with pernicious anemia and other forms of vitamin B12 deficiency are usually identified because of signs and symptoms of anemia, which typically occur before neurologic symptoms. The opponents of folic acid supplementation are concerned that increased folic acid intake in the general population will mask vitamin B12 deficiency and increase the prevalence of neurologic disease in our elderly population. To put this in perspective, approximately 4000 pregnancies, including 2500 live births, in the USA each year are affected by neural tube defects. In contrast, it is estimated that over 10% of the elderly population in the USA, or several million people, are at risk for the neuropsychiatric complications of vitamin B12 deficiency. In acknowledgment of this controversy, the FDA has kept its requirements for folic acid supplementation at a somewhat low level.
HEMATOPOIETIC GROWTH FACTORS
The hematopoietic growth factors are glycoprotein hormones that regulate the proliferation and differentiation of hematopoietic progenitor cells in the bone marrow. The first growth factors to be identified were called colony-stimulating factors because they could stimulate the growth of colonies of various bone marrow progenitor cells in vitro. Many of these growth factors have been purified and cloned, and their effects on hematopoiesis have been extensively studied. Quantities of these growth factors sufficient for clinical use are produced by recombinant DNA technology.
Of the known hematopoietic growth factors, erythropoietin (epoetin alfa), granulocyte colony-stimulating factor (G-CSF), granulocyte-macrophage colony-stimulating factor (GM-CSF), and interleukin-11 (IL-11) are currently in clinical use. Thrombopoietin and other potentially useful hematopoietic factors are still in development.
The hematopoietic growth factors have complex effects on the function of a wide variety of cell types, including nonhematologic cells. Their usefulness in other areas of medicine, particularly as potential anticancer and anti-inflammatory drugs, is being investigated.
ERYTHROPOIETIN
Erythropoietin, a 34-39 kDa glycoprotein, was the first human hematopoietic growth factor to be isolated. It was originally purified from the urine of patients with severe anemia. Recombinant human erythropoietin (rHuEPO, epoetin alfa) is produced in a mammalian cell expression system. After intravenous administration, erythropoietin has a serum half-life of 4-13 hours in patients with chronic renal failure. It is not cleared by dialysis. It is measured in international units (IU). Darbepoetin alfa is a glycosylated form of erythropoietin and differs from it functionally only in having a twofold to threefold longer half-life.
Erythropoietin stimulates erythroid proliferation and differentiation by interacting with specific erythropoietin receptors on red cell progenitors. The erythropoietin receptor is a member of the JAK/STAT superfamily of cytokine receptors that use protein phosphorylation and transcription factor activation to regulate cellular function. Erythropoietin also induces release of reticulocytes from the bone marrow. Endogenous erythropoietin is primarily produced in the kidney. In response to tissue hypoxia, more erythropoietin is produced through an increased rate of transcription of the erythropoietin gene. This results in correction of the anemia, provided that the bone marrow response is not impaired by red cell nutritional deficiency (especially iron deficiency), primary bone marrow disorders (see below), or bone marrow suppression from drugs or chronic diseases.
Normally, an inverse relationship exists between the hematocrit or hemoglobin level and the serum erythropoietin level. Nonanemic individuals have serum erythropoietin levels of less than 20 IU/L. As the hematocrit and hemoglobin levels fall and anemia becomes more severe, the serum erythropoietin level rises exponentially. Patients with moderately severe anemias usually have erythropoietin levels in the 100-500 IU/L range, and patients with severe anemias may have levels of thousands of IU/L. The most important exception to this inverse relationship is in the anemia of chronic renal failure. In patients with renal disease, erythropoietin levels are usually low because the kidneys cannot produce the growth factor. These are the patients most likely to respond to treatment with exogenous erythropoietin. In most primary bone marrow disorders (aplastic anemia, leukemias, myeloproliferative and myelodysplastic disorders, etc) and most nutritional and secondary anemias, endogenous erythropoietin levels are high, so there is less likelihood of a response to exogenous erythropoietin.
Clinical Pharmacology
The availability of erythropoietin has had a significant positive impact for patients with anemia of chronic renal failure. Erythropoietin consistently improves the hematocrit and hemoglobin level and usually eliminates the need for transfusions in these patients. An increase in reticulocyte count is usually observed in about 10 days and an increase in hematocrit and hemoglobin levels in 2-6 weeks. Most patients can maintain a hematocrit of about 35% with erythropoietin doses of 50-150 IU/kg intravenously or subcutaneously three times a week. Failure to respond to erythropoietin is most commonly due to concurrent iron deficiency, which can be corrected by giving oral or parenteral iron. Folate supplementation may also be necessary in some patients.
In selected patients, erythropoietin may also be useful for the treatment of anemia due to primary bone marrow disorders and secondary anemias. This includes patients with aplastic anemia and other bone marrow failure states, myeloproliferative and myelodysplastic disorders, multiple myeloma and perhaps other chronic bone marrow malignancies, and the anemias associated with chronic inflammation, AIDS, and cancer. Patients with these disorders who have disproportionately low serum erythropoietin levels for their degree of anemia are most likely to respond to treatment with this growth factor. Patients with endogenous erythropoietin levels of less than 100 IU/L have the best chance of response, although patients with erythropoietin levels between 100 and 500 IU/L respond occasionally. These patients generally require higher erythropoietin doses (150-300 IU/kg three times a week) to achieve a response, and responses are often incomplete.
Erythropoietin has been used successfully to offset the anemia produced by zidovudine treatment in patients with HIV infection and in the treatment of the anemia of prematurity. It can also be used to accelerate erythropoiesis after phlebotomies for autologous transfusion for elective surgery, or for treatment of iron overload (hemochromatosis).
Erythropoietin is one of the drugs banned by the International Olympic Committee. The use of erythropoietin by athletes is based on their hope that increased red blood cell concentration will increase oxygen delivery and improve performance.
The most common adverse effects of erythropoietin are associated with a rapid increase in hematocrit and hemoglobin and include hypertension and thrombotic complications. These difficulties can be minimized by raising the hematocrit and hemoglobin slowly and by adequately monitoring and treating hypertension. Allergic reactions have been infrequent and mild.
G-CSF and GM-CSF, the two myeloid growth factors currently available for clinical use, were originally purified from cultured human cell lines. Recombinant human G-CSF (rHuG-CSF; filgrastim) is produced in a bacterial expression system. It is a nonglycosylated peptide of 175 amino acids, with a molecular weight of 18 kDa. Recombinant human GM-CSF (rHuGM-CSF; sargramostim) is produced in a yeast expression system. It is a partially glycosylated peptide of 127 amino acids, with three molecular species with molecular weights of 15,500; 15,800; and 19,500. These preparations have serum half-lives of 2-7 hours after intravenous or subcutaneous administration. Pegfilgrastim, a covalent conjugation product of filgrastim and a form of polyethylene glycol, has a much longer serum half-life than recombinant G-CSF, and so it can be injected once per myelosuppressive chemotherapy cycle instead of daily for several days.
The myeloid growth factors stimulate proliferation and differentiation by interacting with specific receptors found on various myeloid progenitor cells. Like the erythropoietin receptor, these receptors are members of the JAK/STAT superfamily. G-CSF stimulates proliferation and differentiation of progenitors already committed to the neutrophil lineage. It also activates the phagocytic activity of mature neutrophils and prolongs their survival in the circulation. G-CSF also has a remarkable ability to mobilize hematopoietic stem cells, ie, to increase their concentration in peripheral blood. This biologic effect underlies a major advance in transplantation¾the use of peripheral blood stem cells (PBSCs) rather than bone marrow stem cells for autologous and allogeneic hematopoietic stem cell transplantation (see below).
GM-CSF has broader biologic actions than G-CSF. It is a multipotential hematopoietic growth factor that stimulates proliferation and differentiation of early and late granulocytic progenitor cells as well as erythroid and megakaryocyte progenitors. Like G-CSF, GM-CSF also stimulates the function of mature neutrophils. GM-CSF acts together with interleukin-2 to stimulate T-cell proliferation and appears to be a locally active factor at the site of inflammation. GM-CSF mobilizes peripheral blood stem cells, but it is significantly less efficacious than G-CSF in this regard.
A. CANCER CHEMOTHERAPY-INDUCED NEUTROPENIA
Neutropenia is a common adverse effect of the cytotoxic drugs used to treat cancer and increases the risk of serious infection in patients receiving chemotherapy. Unlike the treatment of anemia and thrombocytopenia, transfusion of neutropenic patients with granulocytes collected from donors is performed rarely and with limited success. The introduction of G-CSF in 1991 represented a milestone in the treatment of chemotherapy-induced neutropenia. This growth factor dramatically accelerates the rate of neutrophil recovery after dose-intensive myelosuppressive chemotherapy. It reduces the duration of neutropenia and usually raises the nadir count, the lowest neutrophil count seen following a cycle of chemotherapy.
The ability of G-CSF to increase neutrophil counts after myelosuppressive chemotherapy is nearly universal, but its impact on clinical outcomes is more variable. Some clinical trials have shown that G-CSF reduces episodes of febrile neutropenia, requirements for broad-spectrum antibiotics, and days of hospitalization; however, other trials failed to find these favorable outcomes. To date, no clinical trial has shown improved survival in cancer patients treated with G-CSF. Clinical guidelines for the use of G-CSF after cytotoxic chemotherapy recommend reserving G-CSF for patients with a prior episode of febrile neutropenia after cytotoxic chemotherapy, patients receiving dose-intensive chemotherapy, patients at high risk for febrile neutropenia, and patients who are unlikely to survive an episode of febrile neutropenia. Pegfilgrastim is an alternative to G-CSF for prevention of chemotherapy-induced febrile neutropenia. Pegfilgrastim can be administered less frequently, and it may shorten the period of severe neutropenia slightly more than G-CSF.
Like G-CSF and pegfilgrastim, GM-CSF also reduces the duration of neutropenia after cytotoxic chemotherapy. It has been more difficult to show that GM-CSF reduces the incidence of febrile neutropenia, probably because GM-CSF itself can induce fever. In the treatment of chemotherapy-induced neutropenia, G-CSF, 5 mcg/kg/d, or GM-CSF, 250 mcg/m2/d, is usually started within 24-72 hours after completing chemotherapy and is continued until the absolute neutrophil count is > 10,000 cells/u L. Pegfilgrastim is given as a single dose instead of daily injections.
The utility and safety of the myeloid growth factors in the postchemotherapy supportive care of patients with acute myeloid leukemia (AML) have been the subject of a number of clinical trials. Because leukemic cells arise from progenitors whose proliferation and differentiation are normally regulated by hematopoietic growth factors, including GM-CSF and G-CSF, there was concern that myeloid growth factors could stimulate leukemic cell growth and increase the rate of relapse. The results of randomized clinical trials suggest that both G-CSF and GM-CSF are safe following induction and consolidation treatment of myeloid and lymphoblastic leukemia. There has beeo evidence that these growth factors reduce the rate of remission or increase relapse rate. On the contrary, the growth factors accelerate neutrophil recovery and reduce infection rates and days of hospitalization. Both G-CSF and GM-CSF have FDA approval for treatment of patients with AML.
B. OTHER APPLICATIONS
G-CSF and GM-CSF have also proved to be effective in treating the neutropenia associated with congenital neutropenia, cyclic neutropenia, myelodysplasia, and aplastic anemia. Many patients with these disorders respond with a prompt and sometimes dramatic increase ieutrophil count. In some cases, this results in a decrease in the frequency of infections. Because neither G-CSF nor GM-CSF stimulates the formation of erythrocytes and platelets, they are sometimes combined with other growth factors for treatment of pancytopenia.
The myeloid growth factors play an important role in autologous stem cell transplantation for patients undergoing high-dose chemotherapy. High-dose chemotherapy with autologous stem cell support is increasingly used to treat patients with tumors that are resistant to standard doses of chemotherapeutic drugs. The high-dose regimens produce extreme myelosuppression; the myelosuppression is then counteracted by reinfusion of the patient’s own hematopoietic stem cells (which are collected prior to chemotherapy). The administration of G-CSF or GM-CSF early after autologous stem cell transplantation has been shown to reduce the time to engraftment and to recovery from neutropenia in patients receiving stem cells obtained either from bone marrow or from peripheral blood. These effects are seen in patients being treated for lymphoma or for solid tumors. G-CSF and GM-CSF are also used to support patients who have received allogeneic bone marrow transplantation for treatment of hematologic malignancies or bone marrow failure states. In this setting, the growth factors speed the recovery from neutropenia without increasing the incidence of acute graft-versus-host disease.
Perhaps the most important role of the myeloid growth factors in transplantation is for mobilization of peripheral blood stem cells (PBSCs). Stem cells collected from peripheral blood have nearly replaced bone marrow as the hematopoietic preparation used for autologous transplantation, and the use of PBSCs for allogeneic transplantation is also being investigated. The cells can be collected in an outpatient setting with a procedure that avoids much of the risk and discomfort of bone marrow collection, including the need for general anesthesia. In addition, there is evidence that PBSC transplantation results in more rapid engraftment of all hematopoietic cell lineages and in reduced rates of graft failure or delayed platelet recovery.
G-CSF is the cytokine most commonly used for PBSC mobilization because of its increased efficacy and reduced toxicity compared with GM-CSF. To mobilize stem cells, patients or donors are given 5-10 mcg/kg/d subcutaneously for 4 days. On the fifth day, they undergo leukapheresis. The success of PBSC transplantation depends on transfusion of adequate numbers of stem cells. CD34, an antigen present on early progenitor cells and absent from later, committed, cells, is used as a marker for the requisite stem cells. The goal is to reinfuse at least 5 ´ 106 CD34 cells/kg; this number of CD34 cells usually results in prompt and durable engraftment of all cell lineages. It can take several separate leukaphereses to collect enough CD34 cells, especially from older patients and patients who have been exposed to radiation therapy or chemotherapy.
Although the two growth factors have similar effects oeutrophil counts, G-CSF is used more frequently because it is better tolerated. G-CSF can cause bone pain, which clears when the drug is discontinued. GM-CSF can cause more severe side effects, particularly at higher doses. These include fever, malaise, arthralgias, myalgias, and a capillary leak syndrome characterized by peripheral edema and pleural or pericardial effusions. Allergic reactions may occur but are infrequent. Splenic rupture is a rare but serious complication of the use of G-CSF for PBSC.
Interleukin-11 (IL-11) is a 65-85 kDa protein produced by fibroblasts and stromal cells in the bone marrow. Oprelvekin, the recombinant form of interleukin-11 approved for clinical use, is produced by expression in E coli. The half-life of IL-11 is 7-8 hours when the drug is injected subcutaneously.
Thrombopoietin, a 65-85 kDa glycosylated protein, is constitutively expressed by a variety of organs and cell types. Hepatocytes appear to be the major source of human thrombopoietin, and patients with cirrhosis and thrombocytopenia have low serum thrombopoietin levels. Recombinant thrombopoietin is produced by expression in human cells; the recombinant product contains two intramolecular disulfide bonds and a number of carbohydrate side chains.
Interleukin-11 acts through a specific cell surface cytokine receptor to stimulate the growth of multiple lymphoid and myeloid cells. It acts synergistically with other growth factors to stimulate the growth of primitive megakaryocytic progenitors and, most importantly, increases the number of peripheral platelets and neutrophils.
Acting through its own cytokine receptor, thrombopoietin also independently stimulates the growth of primitive megakaryocytic progenitors. In addition, it stimulates mature megakaryocytes and even activates mature platelets to respond to aggregation-inducing stimuli. The critical in vivo role of thrombopoietin has been demonstrated in genetically engineered knockout mice who lack either thrombopoietin or its receptor. These mice have marked thrombocytopenia but do not display anemia or leukopenia.
Patients with thrombocytopenia have a high risk of hemorrhage. Although platelet transfusion is commonly used to treat thrombocytopenia, this procedure can cause adverse reactions in the recipient; furthermore, a significant number of patients fail to exhibit the expected increase in platelet count.
Interleukin-11 is the first growth factor to gain FDA approval for treatment of thrombocytopenia. It is approved for the secondary prevention of thrombocytopenia in patients receiving cytotoxic chemotherapy for treatment of nonmyeloid cancers. Clinical trials show that it reduces the number of platelet transfusions required by patients who experience severe thrombocytopenia after a previous cycle of chemotherapy. Although IL-11 has broad stimulatory effects on hematopoietic cell lineages in vitro, it does not appear to have significant effects on the leukopenia caused by myelosuppressive chemotherapy. Interleukin-11 is given by subcutaneous injection at a dose of 50 mcg/kg/d. It is started 6-24 hours after completion of chemotherapy and continued for 14-21 days or until the platelet count passes the nadir and rises to > 50,000 cells/uL.
Recombinant thrombopoietin is still an investigational agent. The primary focus of current clinical trials is for the treatment of chemotherapy-induced thrombocytopenia and thrombocytopenia accompanying hematologic stem cell transplantation.
The most common adverse effects of interleukin-11 are fatigue, headache, dizziness, and cardiovascular effects. The cardiovascular effects include anemia (due to hemodilution), dyspnea (due to fluid accumulation in the lungs), and transient atrial arrhythmias. Hypokalemia has also been seen in some patients. All of these adverse effects appear to be reversible. In the limited clinical trial data available thus far, recombinant thrombopoietin appears to be well tolerated.
PREPARATIONS AVAILABLE
Abciximab (ReoPro)
Parenteral: 2 mg/mL for IV injection
Alteplase recombinant [t-PA] (Activase*)
Parenteral: 50, 100 mg lyophilized powder to reconstitute for IV injection
Aminocaproic acid (generic, Amicar)
Oral: 500 mg tablets; 250 mg/mL syrup
Parenteral: 250 mg/mL for IV injection
Anisindione (Miradon)
Oral: 50 mg tablets
Antihemophilic factor [factor VIII, AHF] (Alphanate, Bioclate*, Helixate*, Hemofil M, Koate-HP, Kogenate*, Monoclate, Recombinate,* others)
Parenteral: in vials
Anti-inhibitor coagulant complex (Autoplex T, Feiba VH Immuno)
Parenteral: in vials
Antithrombin III (Thrombate III)
Parenteral: 500, 1000 IU powder to reconstitute for IV injection
Aprotinin (Trasylol)
Parenteral: 10,000 units/mL in 100 and 200 mL vials
Argatroban
Parenteral: 100 mg/mL in 2.5 mL vials
Bivalirudin (Angiomax)
Parenteral: 250 mg per vial
Cilostazol (Pletal)
Oral: 50, 100 mg tablets
Clopidogrel (Plavix)
Oral: 75 mg tablets
Coagulation factor VIIa recombinant (NovoSeven*)
Parenteral: 1.2, 4.8 mg powder/vial for IV injection
Dalteparin (Fragmin)
Parenteral: 2500, 5000, 10,000 anti-factor Xa units/0.2 mL for SC injection only
Danaparoid (Orgaran)
Parenteral: 750 anti-Xa units/vial
Dipyridamole (Persantine)
Oral: 25, 50, 75 mg tablets
Oral combination product (Aggrenox): 200 mg extended-release dipyridamole plus 25 mg aspirin
Enoxaparin (low-molecular-weight heparin, Lovenox)
Parenteral: pre-filled, multiple-dose syringes for SC injection only
Eptifibatide (Integrilin)
Parenteral: 0.75, 2 mg/mL for IV infusion
Factor VIIa: see Coagulation factor VIIa recombinant
Factor VIII: see Antihemophilic factor
Factor IX complex, human (AlphaNine SD, Bebulin VH, BeneFix*, Konyne 80, Mononine, Profilnine SD, Proplex T, Proplex SX-T)
Parenteral: in vials
Fondaparinux (Arixtra)
Parenteral: 2.5 mg in 0.5 mL single-dose pre-filled syringes
Heparin sodium (generic, Liquaemin)
Parenteral: 1000, 2000, 2500, 5000, 10,000, 20,000, 40,000 units/mL for injection
Lepirudin (Refludan*)
Parenteral: 50 mg powder for IV injection
Phytonadione [K1] (generic, Mephyton, Aqua-Mephyton)
Oral: 5 mg tablets
Parenteral: 2, 10 mg/mL aqueous colloidal solution or suspension for injection
Protamine (generic)
Parenteral: 10 mg/mL for injection
Reteplase (Retavase*)
Parenteral: 10.8 IU powder for injection
Streptokinase (Streptase)
Parenteral: 250,000, 750,000, 1,500,000 IU per vial powders to reconstitute for injection
Tenecteplase (TNKase*)
Parenteral: 50 mg powder for injection
Ticlopidine (Ticlid)
Oral: 250 mg tablets
Tinzaparin (Innohep)
Parenteral: 20,000 anti-Xa units/mL for subcutaneous injection only
Tirofiban (Aggrastat)
Parenteral: 50, 250 mcg/mL for IV infusion
Tranexamic acid (Cyklokapron)
Oral: 500 mg tablets
Parenteral: 100 mg/mL for IV infusion
Urokinase (Abbokinase)
Parenteral: 250,000 IU per vial for systemic use
Warfarin (generic, Coumadin)
Oral: 1, 2, 2.5, 3, 4, 5, 6, 7.5, 10 mg tablets
Darbepoetin alfa (Aranesp)
Parenteral: 25, 40, 60, 100, 200, 300, 500 mcg/mL for IV or SC injection
Deferasirox (Exjade)
Oral: 125, 250, 500 mg tablets
Deferoxamine (generic, Desferal)
Parenteral: 500, 2000 mg vials for IM, SC, or IV injection
Epoetin alfa (erythropoietin, EPO) (Epogen, Procrit)
Parenteral: 2000, 3000, 4000, 10000, 20000, 40000 IU/mL vials for IV or SC injection
Filgrastim (G-CSF) (Neupogen)
Parenteral: 300 mcg vials for IV or SC injection
Folic acid (folacin, pteroylglutamic acid) (generic)
Oral: 0.4, 0.8, 1 mg tablets
Parenteral: 5 mg/mL for injection
Iron (generic)
Oral
Parenteral (Iron dextran) (InFeD, DexFerrum): 50 mg elemental iron/mL
Parenteral (Sodium ferric gluconate complex) (Ferrlecit): 12.5 mg elemental iron/mL
Parenteral (Iron sucrose)(Venofer): 20 mg elemental iron/mL
Oprelvekin (interleukin-11) (Neumega)
Parenteral: 5 mg vials for SC injection
Pegfilgrastim (Neulasta)
Parenteral: 10 mg/mL solution in single-dose syringe
Sargramostim (GM-CSF) (Leukine)
Parenteral: 250, 500 mcg vials for IV infusion
Vitamin B12 (generic cyanocobalamin or hydroxocobalamin)
Oral (cyanocobalamin): 100, 500, 1000, 5000 mcg tablets, 100, 250, 500 mcg lozenges
Nasal (Nascobal): 5000 mcg/mL (500 mcg/spray)
Parenteral (cyanocobalamin): 100, 1000 mcg/mL for IM or SC injection
Parenteral (hydroxocobalamin): 1000 mcg/mL for IM injection only
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