Katherine A. Thompson

The relationship between debrisoquine metabolic phenotype and the pharmacokinetics and pharmacodynamics of propafenone was studied in 28 patients with chronic ventricular arrhythmias (22 extensive metabolizers [EMs] and six poor metabolizers [PMs] of debrisoquine). EMs were characterized by a shorter propafenone elimination half-life (5.5 +/- 2.1 vs 17.2 +/- 8.0, p less than .001), lower average plasma concentration (Cp) (1.1 +/- 0.6 vs 2.5 +/- 0.5 ng/ml/mg daily dosage, p less than .001), and higher oral clearance (1115 +/- 1238 vs 264 +/- 48 ml/min, p less than .001). The active metabolite 5-hydroxypropafenone, assayed in 12 patients, was identified in nine of 10 EMs but in neither of the PMs. A lower incidence of central nervous system side effects was noted in EMs (14% vs 67%, p less than .01). The magnitude of QRS widening at any given propafenone Cp was greater in EMs than PMs. There was no significant difference between EMs and PMs in effective propafenone dose or frequency of antiarrhythmic response. Inhibition of debrisoquine 4-hydroxylation by propafenone was demonstrated both in vivo and in a human liver microsomal system in vitro. We conclude that propafenone is metabolized via the same cytochrome P-450 responsible for debrisoquine's 4-hydroxylation, and that its pharmacokinetics and concentration-response relationships and the incidence of central nervous system side effects are different in patients of different debrisoquine metabolic phenotype.

Astrocytes are the most numerous cell type in the brain, and their physiological roles are essential for normal brain function. Studies of post-mortem brain tissue samples from individuals with AIDS have revealed that a small proportion of astrocytes are infected by HIV-1 which is linked to the development of HIV-associated dementia (HIVD), a frequent clinical manifestation of HIV-1 disease affecting up to 20% of infected adults. However, astrocyte infection by HIV-1 in vivo is generally non-productive, and can only be readily detected by sensitive techniques that detect HIV-1 RNA or proviral DNA. Similarly, primary astrocyte cultures and astrocytic cell lines can be permissive to infection by HIV-1 strains, but are refractory to efficient HIV-1 expression. In efforts to delineate the molecular mechanisms underlying the "restricted" infection, several studies have demonstrated that efficient HIV-1 replication is blocked in astrocytes at different steps of the virus life cycle, including virus entry, reverse transcription, nucleocytoplasmic HIV-1 RNA transport, translation of viral RNA, and maturation of progeny virions. However, the relative importance of each of these possible replication blocks in restricting HIV-1 replication in astrocytes is unclear. Moreover, how restricted astrocyte infection contributes to the development of HIVD is unknown. This review surveys the current in vitro models of restricted HIV-1 replication in astrocytes, and provides an analysis of the available evidence supporting a role for astrocyte infection in the pathogenesis of HIVD. A greater understanding of the fate of HIV-1 in astrocytes may assist in the identification of viral reservoirs in the central nervous system, novel therapies for the treatment of HIVD, and also novel strategies to suppress HIV-1 replication in CD4+ cells of the immune system.