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Journal of Virology, September 2001, p. 7925-7933, Vol. 75, No. 17
0022-538X/01/$04.00+0 DOI: 10.1128/JVI.75.17.7925-7933.2001
Copyright © 2001, American Society for Microbiology. All rights reserved.
Highly Productive Infection with Pseudotyped Human
Immunodeficiency Virus Type 1 (HIV-1) Indicates No Intracellular
Restrictions to HIV-1 Replication in Primary Human Astrocytes
Mario
Canki,1
Janice Ngee Foong
Thai,1
Wei
Chao,1
Anuja
Ghorpade,2
Mary Jane
Potash,1 and
David J.
Volsky1,*
Division of Molecular Virology, St.
Luke's-Roosevelt Hospital Center and Columbia University, New
York, New York 10019,1 and Center for
Neurovirology and Neurodegenerative Disorders, University of
Nebraska Medical Center, Omana, Nebraska 681982
Received 12 March 2001/Accepted 24 May 2001
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ABSTRACT |
Human astrocytes can be infected with human immunodeficiency virus
type 1 (HIV-1) in vitro and in vivo, but, in contrast to T lymphocytes
and macrophages, virus expression is inefficient. To investigate the
HIV-1 life cycle in human fetal astrocytes, we infected cells with
HIV-1 pseudotyped with envelope glycoproteins of either amphotropic
murine leukemia virus or vesicular stomatitis virus. Infection by both
pseudotypes was productive and long lasting and reached a peak of 68%
infected cells and 1.7 µg of viral p24 per ml of culture supernatant
7 days after virus inoculation and then continued with gradually
declining levels of virus expression through 7 weeks of follow-up. This
contrasted with less than 0.1% HIV-1 antigen-positive cells and 400 pg
of extracellular p24 per ml at the peak of astrocyte infection with
native HIV-1. Cell viability and growth kinetics were similar in
infected and control cells. Northern blot analysis revealed the
presence of major HIV-1 RNA species of 9, 4, and 2 kb in astrocytes
exposed to pseudotyped (but not wild-type) HIV-1 at 2, 14, and 28 days
after infection. Consistent with productive infection, the 9- and 4-kb
viral transcripts in astrocytes infected by pseudotyped HIV-1 were as
abundant as the 2-kb mRNA during 4 weeks of follow-up, and both
structural and regulatory viral proteins were detected in infected
cells by immunoblotting or cell staining. The progeny virus released by
these cells was infectious. These results indicate that the major
barrier to HIV-1 infection of primary astrocytes is at virus entry and
that astrocytes have no intrinsic intracellular restriction to
efficient HIV-1 replication.
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INTRODUCTION |
The central nervous system (CNS) is
a major target for human immunodeficiency virus type 1 (HIV-1)
infection. HIV-1 enters the CNS early after systemic infection and
persists there for life (20, 26, 30). About 30% of AIDS
patients develop prominent cognitive, motor, and behavioral
manifestations known as HIV-1 encephalopathy, AIDS dementia complex, or
HIV-associated dementia (45, 48, 49, 60). HIV-1 is
considered the principal etiologic agent of this disorder (22,
39, 45), but the mechanism of HIV-1-induced neuropathogenesis is
unknown. The virus can be found in the brain in infiltrating
macrophages, microglial cells, astrocytes, oligodendrocytes, and brain
endothelial cells but only infrequently in neurons (53, 57, 67,
68, 73), indicating that the observed neuronal damage cannot be
directly attributed to HIV-1 replication in these cells. Macrophages
and microglial cells are considered to be the primary source of HIV-1
replication within the CNS, and HIV-1 strains isolated from the CNS
generally exhibit R5 or macrophage-tropic characteristics, indicating
that such strains predominate in the brain (14, 31, 34, 40, 57, 67, 68, 73). Productive infection of macrophages and microglial cells is believed to contribute to neuropathogenesis through secretion of viral (gp120, Tat, and Nef) and cellular (cytokines, chemokines, and
nitric oxide) neurotoxic products (reviewed in references 35 and
41). However, HIV-1 infection of these cells may not be
sufficient for the development of neuropathology. Studies in a macaque
model of simian immunodeficiency virus (SIV) encephalitis indicate, for
example, that there is no direct correlation between macrophage tropism
and neuroinvasiveness or neurovirulence of SIV (43, 66).
Recent studies have shown that neurons express CXCR4 (23,
29) and that HIV-1 strains which utilize CXCR4 for entry can
induce signal transduction and apoptosis in neurons (75)
specifically through these receptors (52, 75). We have shown that some primary HIV-1 isolates obtained from vitreous from AIDS
patients with cytomegalovirus retinitis can infect astrocytes and T
lymphocytes but not macrophages (11). Thus, multiple HIV-1 strains and brain cell types infected with the virus may contribute to
HIV-1-mediated neuropathogenesis.
Recently, attention has been directed toward the potential role of
astrocytes in HIV-1 neuropathogenesis (9, 19). Astrocytes are critical for brain homeostasis and for responses to pathogens and
brain injury (8, 15, 19, 71), and defects in astrocyte functions may lead to neurodegeneration (54). Astrocytes
also are a major target for HIV-1 infection in the brain. Depending on
methodology of HIV-1 detection, stage of brain disease, and brain
region analyzed, reports have shown that anywhere from 0 to 20% of
astrocytes may carry the HIV-1 genome in vivo (5, 10, 25, 51, 53,
57, 67, 68), with larger-scale surveys indicating a frequency of
up to 1% (67). Considering that the number of astrocytes
in the brain ranges between 4 × 1011 and 2 × 1012 cells (55), the total number of
HIV-1-infected astrocytes in vivo may be substantial.
We are interested in the course of HIV-1 infection of astrocytes and
potential effects of that infection on astrocyte function. In contrast
to productive and cytopathic infection in T cells and macrophages
(reviewed in reference 39), HIV-1 infection of astrocytes
is inefficient, of low productivity, and generally noncytopathic
(11, 13, 21, 24, 36, 47, 65, 69, 70). We and others have
estimated that only about 1% of human fetal astrocytes express virus
at the peak of infection (7, 28). On this basis, there is
general agreement that infection or transfection of astrocytes produces
a transient burst of viral replication, which diminishes to low levels
of virus expression or latency (7, 11, 56, 58, 59, 69,
70). The reasons behind this limited infection are not well
understood, but they could include inefficient virus entry,
intracellular restrictions to virus replication, or a combination of
the two. Intracellular restrictions are suggested by findings showing
that infected astrocytes contain mostly viral regulatory proteins and
transcripts coding for these products but only low levels of viral
structural proteins (57, 67, 69, 70). Studies indicate
that this restriction may result from limited expression of HIV-1 RNA
encoding the major structural proteins (69), possibly due
to inefficient Rev function (42, 50). Inefficient HIV-1
production in certain glioma cell lines has also been correlated with
defects in processing of HIV-1 gp160 envelope glycoprotein
(58) and inefficient translation of HIV-1 structural
proteins (24). Block at HIV-1 entry into astrocytes is
implied by the absence of surface CD4 expression by the cells
(13). In some but not all glial cell lines (17, 27), stable expression of CD4 permits high-level, productive infection by HIV-1 (59, 61, 72, 74). Transient
transfection of HIV-1 DNA into astrocytes or cocultivation with
HIV-1-infected cells also permits more efficient virus replication than
does exposure to cell-free virus (7, 21, 47, 65, 69), and some glioma cells stably transfected with HIV-1 DNA replicate virus at
high levels (21, 59). Together, these studies suggest that
virus entry is a major limiting step of HIV-1 infection in astrocytes.
We reported previously that HTB148 glioma cells which were stably
transfected to express surface CD4 are susceptible to efficient HIV-1
infection (72). In the present work, we applied a slightly different strategy to investigate the life cycle of HIV-1 in primary human astrocytes. Rather than confer expression of CD4 on primary astrocytes, which was technically difficult, we extended HIV-1 tropism
by pseudotyping, that is, endowing native HIV-1 with heterologous envelope glycoproteins that bind commonly expressed cellular receptors. Vesicular stomatitis virus (VSV) G protein mediates entry via an
endocytic pathway (44), and amphotropic murine leukemia
virus (MLV) glycoprotein mediates virus-cell membrane fusion, mimicking the entry of HIV-1 (46). HIV-1 pseudotyped with either VSV
or MLV envelope glycoproteins efficiently infects CD4-negative cells (2, 3, 6, 64). Here, HIV-1 NL4-3 was pseudotyped with VSV
or amphotropic MLV envelopes by cotransfection of intact NL4-3 DNA and
either a VSV or MLV envelope expression vector, yielding VSV/NL4-3 and
MLV/NL4-3, respectively. We compared infection of primary human fetal
astrocytes by native NL4-3 to infection by pseudotyped HIV-1. We found
that in contrast to native NL4-3, both VSV/NL4-3 and MLV/NL4-3 were
able to productively infect the majority of astrocytes, permitting
quantitative analysis of the viral life cycle in these cells by Western
and Northern blotting and immunofluorescent staining of cells with
anti-HIV sera. Our results suggest that primary astrocytes pose no
fundamental intracellular block to HIV-1 replication. These results
introduce a model system of efficient HIV-1 infection of primary
astrocytes for studies of the course of the HIV-1 life cycle in these cells.
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MATERIALS AND METHODS |
Cells.
Fetal astrocytes were isolated from second-trimester
(gestational age, 16-19 weeks) human fetal brains obtained from
elective abortions in full compliance with National Institutes of
Health (NIH) guidelines, as previously described (11, 75).
Highly homogenous preparations of astrocytes were obtained using
high-density culture conditions in the absence of growth factors in F12
Dulbecco's modified Eagle's medium (GIBCO-BRL, Gaithersburg, Md.)
containing 10% fetal bovine serum, penicillin, streptomycin, and
gentamicin (11, 75). Subsequently, the cells were
maintained in this medium at 2 × 104 to 5 × 104 cells/cm2 and subcultured weekly up to six
times. For each experiment, a single batch of astrocytes of the same
gestational age and passage was used. Cultures were regularly monitored
for expression of the astrocytic marker glial fibrillary acidic protein
(GFAP) and either HAM56 or CD68 to identify cells of
monocyte/macrophage lineage. Only cultures that contained
99%
GFAP-positive cells and rare or no detectable HAM56- or CD68-positive
cells were used in our experiments (75).
HIV-1 molecular clones, envelope expression vectors, and
generation of pseudotyped HIV-1.
The HIV-1 molecular clones used
were NL4-3, which expresses all known HIV-1 proteins (1),
and NL-P1, an NL4-3 derivative carrying the marker gene human placental
alkaline phosphatase (PLAP) inserted next to Nef (18). The
VSV G expression vector pL-VSV-G was obtained from M. Emerman; it
contains a VSV G insert in the pcDNA expression vector modified by
replacing the cytomegalovirus promoter with the HIV-1 long terminal
repeat (6). The amphotropic MLV envelope expression vector
SV-A-MLV-Env was obtained from D. Littman; envelope expression in this
vector is driven by the MLV long terminal repeat (38).
High-titer virus stocks were produced in 293T human embryonic kidney
cells transfected with the respective DNA by calcium phosphate
precipitation (4). To generate pseudotyped virus, 1.5 × 106 293T cells cultured in 10-cm plates were
cotransfected with 10 µg of HIV-1 clone DNA and 15 µg of VSV or MLV
envelope expression plasmid DNA, a ratio of DNAs found to yield the
highest HIV-1 infectious titers in our hands. For native HIV-1
production, 1.5 × 106 293T cells were transfected
with 15 µg of NL4-3 or NL-P1 DNA. 293T culture supernatants were
harvested 72 h after transfection, filtered through a
0.45-µm-pore-size Millipore filter, and stored at
80°C until use.
Cell-free viral stock was tested for HIV-1 p24 core antigen content by
enzyme-linked immunosorbent assay (ELISA) using the HIV-1 Ag kit as
specified by the manufacturer (Coulter, Hialeah, Fla) and for titers of
infectious virus by multinuclear activation of a
-galactosidase
indicator (MAGI) assay (33). Culture supernatants
contained 1 to 2 µg of viral p24 protein per ml and 1 × 106 to 2 × 106 infectious units (IU) per
ml. In our hands, a multiplicity of infection of 1 for CD4-positive T
cells is equivalent to approximately 1 pg of viral p24 per cell
(21, 59).
Cell infection and analysis of HIV-1 expression by p24 ELISA and
IF.
Confluent cultures of human fetal astrocytes were infected
with native or pseudotyped HIV-1 at 1 pg of p24 per cell overnight and
washed five times with Hanks balanced salt solution (GIBCO-BRL) before
being returned to culture. At the indicated times after infection,
culture supernatants were tested for the levels of HIV-1 p24 antigen by
p24 ELISA and cells were removed, spotted on glass slides, fixed in
acetone, and stained with AIDS patient serum to detect HIV-1 antigens
by indirect immunofluorescence (IF). Astrocytes infected with NL-P1
virus were also stained for PLAP by IF using mouse anti-alkaline
phosphatase antibody (Serotec, Raleigh, N.C.). GFAP-positive astrocytes
were detected by IF staining using rabbit anti-GFAP (DAKO Corp.,
Carpinteria, Calif.). All secondary antibodies were conjugated with
fluorescein isothiocyanate, positive cells were visualized under an
Olympus BH-2 fluorescence microscope, and at least 200 cells were
counted. HIV-1 antigen and GFAP staining were also performed on cells
cultured on coverslips, plated, and infected under the same conditions
as in large-scale cultures. The results were similar to those obtained
with cells removed by trypsinization from large-scale cultures.
HIV-1 protein analysis by immunoblotting.
Cells were counted
and lysed in a buffer containing 1% Triton X-100, 0.1% sodium dodecyl
sulfate (SDS), 1% sodium deoxycholate, 5 mM iodoacetamide, and 0.2 U
of phenylmethylsulfonyl fluoride per ml, and cell lysates corresponding
to equivalent numbers of cells were resolved by SDS-polyacrylamide gel
electrophoresis on 4 to 15% polyacrylamide ready gels (Bio-Rad,
Hercules, Calif.) and transferred onto a 0.2-µm-pore-size Trans-Blot
nitrocellulose membrane (Bio-Rad). The membranes were incubated in 5%
(wt/vol) skim milk in T-PBS (0.1% polyoxyethyline-sorbitan monolaurate in phosphate-buffered saline [PBS]) and then stained with indicated primary antibodies followed by horseradish peroxidase-conjugated second
antibody. Protein bands were visualized on X-ray film after a
luminescence reaction using the ECL kit (Amersham, Arlington Heights,
IU.). Samples were standardized by their
-tubulin content prior to
final evaluations.
Viral RNA analysis by Northern blot hybridization.
Total
cellular RNA was isolated with TRIzol (GIBCO-BRL) as specified by the
manufacturer, samples were standardized by their optical density at 262 nm, and 20 µg of RNA per lane was resolved by electrophoresis through
an agarose-formaldehyde gel (1% agarose, 2.2 M formaldehyde, 10%
[vol/vol] 10× MOPS [0.4 M MOPS, pH7; 0.1 M sodium acetate, 0.01 M
EDTA]) in 1× MOPS (morpholinepropanesulfonic acid) running buffer
using a standard procedure (4). The gels were denatured in
0.05 M NaOH-1.5 M NaCl for 30 min, neutralized in 0.5 M Tris-Cl
(pH7.4) to 1.5M NaCl for 20 min, and washed in 20× SSC (1× SSC in
0.15 M NaCl plus 0.015 M sodium citrate) for 45 min, and RNA was
blotted onto a 0.45-µm-pore-size NYTRAN SPC membrane (Schleicher & Schuell, Keene, N.H.) and hybridized with an 8.9-kb SacI
proviral DNA fragment derived from NL4-3 (58) labeled with
[
-32P]dCTP using the RadPrime DNA Labeling System
(GIBCO-BRL). Hybridization was carried out overnight at 42°C in a
buffer containing 6× SSC, 5× Denhardt's reagent, 0.5% SDS, 100 µg
of salmon sperm DNA per ml, and 50% formaldehyde; the membranes were
then washed under stringent conditions and analyzed by autoradiography.
Other analytical procedures and reagents.
Cell viability was
determined by trypan blue exclusion counting. The biological activity
of progeny virus made in astrocytes was determined by testing virus
infectivity in the MAGI assay (33). The following reagents
used were obtained through the AIDS Research and Reference Reagent
Program, Division of AIDS, National Institute of Allergy and Infectious
Diseases, NIH: hybridoma cells producing monoclonal anti-Gag HIV-1 p24
(obtained from Bruce Chesebro and Hardy Chen) (183-H12-5C; 1513)
(14), mouse monoclonal anti HIV-1 V3 (obtained from Jon
Laman) (IIIB-V3-13; 1727) (37), and monoclonal anti-Nef
antiserum (obtained from Ronald Swanstrom) (HIV-1 Nef antiserum; 2949)
(62). The monoclonal
-tubulin antibody was purchased
from Sigma (St. Louis, Mo.).
 |
RESULTS |
HIV-1 pseudotyped with VSV-G or MLV envelope causes lasting and
highly productive infection in primary astrocytes.
Infection of
primary human astrocytes with native HIV-1 in vitro is inefficient,
with fewer than 1% of cells expressing viral antigens and virus
production being low (7, 28, 70). We first tested whether
exposure of astrocytes to HIV-1 pseudotyped with VSV G or MLV envelope,
which bypasses the natural mode of HIV-1 entry into these cells, can
increase the susceptibility of astrocytes to HIV-1 infection and
replication. Astrocytes were isolated from second-trimester human fetal
brains and cultured under conditions that minimize the growth of
nonastrocytic brain cells, as previously described (7, 11,
75). The cultures were regularly evaluated by IF staining for
expression of GFAP, an astrocytic marker, and HAM56 or CD68, to detect
macrophages and microglial cells. Cells found to contain
99%
GFAP-positive cells and no detectable HAM56 and CD68 signals were used
in further experiments. Staining of a representative culture for GFAP
is shown in Fig. 1A. Astrocytes were
exposed overnight to native NL4-3 or NL4-3 pseudotyped with MLV
(MLV/NL4-3) or VSV-G (VSV/NL4-3) envelope glycoproteins at 1 pg of
viral p24 per cell and tested at the indicated time intervals for
expression of cell-associated HIV-1 antigens by IF staining (Fig. 1C
and D) and for levels of viral p24 in culture supernatants by p24 ELISA
(Fig. 2A). In parallel, cultures were monitored for cell growth
kinetics and viability (Fig. 2B). As determined by IF staining,
expression of cell-associated HIV-1 antigens peaked on day 7, with 68 and 34% of cells positive after VSV/NL4-3 and MLV/NL4-3 infection,
respectively (Fig. 2A). Subsequently,
virus expression declined at a similar rate in both VSV/NL4-3- and
MLV/NL4-3-infected cultures, but, remarkably, viral proteins were still
detected by IF in 8 to 9% of cells 7 weeks after infection (Fig. 2A).
Figures 1C and D show examples of IF staining of HIV-1-infected
astrocytes from this experiment. Consistent with IF results, parallel
measurements of HIV-1 p24 antigen levels in culture supernatants
revealed a peak of p24 production on day 7 at 1.7 µg of p24/ml for
VSV/NL4-3-infected and 0.48 µg of p24/ml for MLV/NL4-3-infected
astrocytes, followed by a gradual decline to approximately 100 ng/ml by
7 weeks after infection (Fig. 2A). As measured by IF staining and p24
antigen production, infection of astrocytes with VSV/NL4-3 was more
efficient than infection with MLV/NL4-3 at the same dose (Fig. 2). The
reasons for this difference are not clear, but similar results were
noted in studies using other target cells (3). Infection
of astrocytes with pseudotyped HIV-1 was virus dose dependent in a
linear fashion as measured by IF and p24 antigen production (data not
shown). In contrast to astrocytes infected with pseudotyped HIV-1 and consistent with previous studies (7, 70), only limited
infection was observed in cells exposed to native NL4-3, with few
astrocytes staining positive for HIV-1 antigens by IF and less than 400 pg of p24/ml being detectable in culture supernatants at the peak of
infection (Fig. 2A). Similar results were obtained in more than 20 experiments using different batches of astrocytes and HIV-1. We
conclude that use of HIV-1 pseudotyped with viral envelopes of a broad
cellular tropism permits a rapid, highly productive, and long-lasting
infection of the majority of astrocytes in culture.

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FIG. 1.
GFAP expression by human fetal astrocytes and IF
detection of HIV-1 antigens in infected astrocytes. (A and B)
Uninfected human fetal astrocytes (16 weeks of gestational age, third
passage) were grown on glass chamber slides and stained with anti-GFAP
antibody (A) or irrelevant control antibody (B). (C to E)
VSV/NL4-3-infected astrocytes from the experiment described in the
legend to Fig. 2 were harvested, fixed, and stained for HIV-1 antigens
by IF 7 days (C) and 28 days (D) after infection; cells harvested 7 days after infection, stained with an irrelevant serum, are also shown
(E). Photographs were taken using an Olympus BH-2 fluorescence
microscope. Magnification, ×100.
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FIG. 2.
Expression of HIV-1 antigens, viability, and growth
kinetics in fetal astrocytes infected with native and pseudotyped
HIV-1. (A) Astrocyte cultures were infected with VSV/NL4-3, MLV/NL4-3,
or NL4-3 as indicated and monitored for HIV-1-specific antigens
expression by IF staining with AIDS sera and fluorescein
isothiocyarate-conjugated second antibody (left panel) or by production
of p24 in cell supernatants (right panel). The proportion of
IF-positive cells was determined by counting at least 200 cells each in
three different fields under ×20 magnification, using an Olympus BH-2
fluorescence microscope. (B) At the indicated times after infection,
total cell numbers and total viable-cell numbers per system (×1,000)
were determined as described in Materials and Methods.
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The level of HIV-1 expression in astrocytes infected with VSV/NL4-3 or
MLV/NL4-3 (Fig.
1 and
2) was similar to and often higher
than the level
we usually observed in HIV-1-infected peripheral
blood lymphocytes
(PBL) and macrophages (
16,
63). Normally,
HIV-1
replication in PBL is cytopathic while infected macrophages
can produce
large quantities of virus for extended periods without
cytolysis (for a
review, see: reference
39). To determine whether
astrocytes survive productive HIV-1 infection, we tested cell
growth
kinetics and viability in parallel with virus expression
measurements
in the experiment summarized in Fig.
2. These results
are shown in Fig.
2B. In all systems, i.e., uninfected cells,
NL4-3-infected cells that
produce minimal amounts of virus, and
cells productively infected with
VSV/NL4-3 or MLV/NL4-3, astrocytes
proliferated and remained fully
viable throughout 7 weeks of follow-up
(Fig.
2B). The total number of
astrocytes infected with VSV/NL4-3
was smaller at the end of the
experiment than the numbers of control
or other infected cells (Fig.
2B), possibly because of initial
cell damage from membrane fusion
caused by the VSV-G protein (
6).
A similar cell
proliferation rate in all culture systems over
a prolonged period
indicates that HIV-1 infection of astrocytes,
whether of low
productivity (with native NL4-3) or of high productivity
(with
pseudotyped NL4-3), is largely
noncytolytic.
Astrocytes infected with pseudotyped HIV-1 efficiently transcribe
viral mRNA and persistently express viral structural proteins.
Previous studies of HIV-1 expression in primary astrocytes and glioma
cell lines produced conflicting results, with some authors suggesting
restricted expression of viral RNA or proteins (24, 50,
69) and others showing no intrinsic intracellular restrictions to efficient viral replication (7, 58, 74). Efficient
infection of astrocytes with pseudotyped HIV-1 (Fig. 1 and 2) permitted us to evaluate HIV-1 RNA transcription and protein expression in these
cells by standard biochemical techniques of Northern blot hybridization
and immunoblotting, respectively (see Fig. 3 and 4). To determine the
steady-state levels of the major HIV-1 mRNA species relative to each
other at different times after infection, astrocytes were infected with
VSV/NL4-3, MLV/NL4-3, or NL4-3 as described above and total cellular
RNA was isolated and subjected to Northern blot analysis with an
HIV-1-specific probe on days 2, 14, and 28 after infection (Fig.
3). As expected because of low virus
production, viral RNA was undetectable by this method in astrocytes
infected with native NL4-3 (Fig. 3). In contrast, the three major HIV-1
mRNA species of 9, 4, and 2 kb were clearly detectable in astrocytes
productively infected with VSV/NL4-3 or MLV/NL4-3 at all the time
points tested, including 4 weeks after infection (Fig. 3). The 9-kb RNA
was a predominant viral RNA species 2 and 14 days after infection and
was present at about a 1:1 ratio with respect to the 4-kb HIV-1 RNA at
4 weeks after infection (Fig. 3). The 2-kb viral RNA was the least
abundant species at all three time points. The consistent presence of
9-kb viral RNA in pseudotyped HIV-1-infected astrocytes correlated well
with efficient virus production over the same period, as indicated by
p24 levels in culture supernatants (Fig. 2). T cells productively
infected by HIV-1 and tested as positive control also contained the
three major HIV-1 RNA species (Fig. 3). Similar results were obtained
in three independent experiments. We conclude that in our model system
of HIV-1 infection of primary astrocytes, there is no selective defect
in steady-state expression of the 9- and 4-kb HIV-1 mRNA or,
conversely, that the 2-kb viral mRNA does not predominate over the
course of infection.

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FIG. 3.
Northern blot analysis of HIV-1 RNA expression in
astrocytes infected with pseudotyped HIV-1. Astrocytes were infected
with VSV/NL4-3, MLV/NL4-3, or NL4-3 and analyzed for HIV-1 RNA by
Northern blotting 2, 14, and 28 days after infection as described in
Materials and Methods. A total of 20 µg of total-cell RNA was loaded
per lane. Samples from day 2 and 14 were exposed for 24 h, and
samples from day 28 were exposed for 14 days. NL4-3-infected H9 cells
were analyzed in parallel as positive controls; the samples were
exposed for 24 h.
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To identify some of the HIV-1 structural and regulatory proteins
expressed in astrocytes, cells were infected with pseudotyped
NL4-3 or
NL-P1, harvested at the peak of infection (7 days) and
during the
decline of viral replication (35 days), and analyzed
by Western
blotting for the presence of the HIV-1 regulatory protein
Nef and viral
structural proteins Env and Gag (Fig.
4).
NL-P1
is a reporter HIV-1 which expresses human PLAP (
18)
and which
is used in the kinetics studies described below (see Fig.
5).
HIV-1 Gag was detected using a monoclonal anti-p24 antibody that
recognizes both mature p24 and Gag p55 polyprotein; the anti-V3
antibody used detects gp160 and gp120 envelope glycoproteins but
not
gp41. The samples were standardized by measurement of their

-tubulin
content. All the proteins tested were readily detected
in astrocytes 7 days after infection with pseudotyped HIV-1 (Fig.
4A to C). As
expected, no viral proteins could be detected in
NL4-3-infected
astrocytes by this method (data not shown). Consistent
with the less
efficient infection of astrocytes by MLV/NL4-3 than
by VSV/NL4-3 (Fig.
2), the protein signals in the MLV/NL4-3 lanes
in Fig.
4 were weaker
than in other systems. The stronger Nef
protein signal in the VSV/NL-P1
lane in Fig.
4 compared to corresponding
bands in VSV/NL4-3 and
MLV/NL4-3 lanes was probably due to overexpression
of Nef by NL-P1, in
which Nef (as well as PLAP) is expressed under
the control of a
picornavirus element, the internal ribosome entry
site, allowing
cap-independent initiation of translation (
12,
18).
Infected cells tested with an anti-Env antibody contained
both the
HIV-1 envelope precursor glycopolyprotein gp160 and the
processed
envelope protein gp120 (Fig.
4B). We also detected the
envelope
glycoprotein gp41 by using an anti-gp41 antibody (data
not shown).
These results indicate that primary astrocytes express
the cellular
enzymes required for gp160 processing into component
envelope proteins.
Notably, the Gag p55 polyprotein and mature
p24 core protein were also
readily detected 35 days after infection
(Fig.
4D), indicating that in
our system, the observed gradual
decline in HIV-1 production in
astrocytes over time can not be
attributed to a shutoff of Gag
polyprotein processing. Similar
results were obtained in three
independent experiments. The results
of Western blot analysis (Fig.
4)
are consistent with those of
IF and extracellular p24 assays (Fig.
2),
which also indicated
long-term productive HIV-1 infection in
astrocytes. We conclude
that in our system, human primary astrocytes
permit the expression
of HIV-1 structural proteins for an extended
period after infection.

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FIG. 4.
Western blot analysis of Gag, gp120, and Nef proteins by
infected astrocytes. Astrocytes were infected with HIV-1 as indicated
and tested for HIV-1 proteins by immunoblotting as described in
Materials and Methods. All systems were normalized first by measurement
of the -tubulin content. (A and D) Gag levels 7 and 35 days after
infection, respectively. (B and C) gp120 and Nef protein levels 7 days
after infection. Panel D contains four times more protein per lane than
does panel A. Mock indicates uninfected astrocytes, and infected and
uninfected PBL are shown for comparison. The results are representative
of three experiments.
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Previous studies using primary astrocytes transfected with HIV-1 DNA in
vitro indicated that an initial productive phase of
viral replication
in that system was followed by a more restrictive
phase characterized
by predominant expression of doubly spliced
2-kb transcripts encoding
viral Nef, Tat, and Rev (
69). We have
not seen such
preferential expression (Fig.
3), but in our system
virus production
also declines over time (Fig.
2). In the study
whose results are shown
in Fig.
5, we used MLV/NL-P1 as a
reporter
virus to investigate whether the proportion of infected
astrocytes
expressing viral structural proteins (synthesized from 9- and
4-kb RNAs) declines at a similar rate to the proportion of cells
expressing a 2-kb viral RNA product, here represented by the PLAP
marker protein expressed from a doubly spliced Nef mRNA
(
12).
Astrocytes were infected with MLV/NL-P1 and tested
at the indicated
times for expression of HIV-1 antigens and PLAP by IF
staining
(Fig.
5). HIV-1 antigens were detected using AIDS serum that
recognizes
mostly viral structural proteins (data not shown), and PLAP
was
detected with anti-PLAP antibody. Overall, the kinetics of
expression
of HIV-1 proteins and PLAP in MLV/NL-P1-infected astrocytes
followed
the pattern described above for VSV/NL4-3 and MLV/NL4-3 (Fig.
2): the infection peaked on day 7 with about 30% positive cells
for
both HIV-1 proteins and PLAP, and the overall proportions
of
IF-positive cells declined gradually to lower but detectable
levels
throughout the 7 weeks of follow-up (Fig.
5). The ratio
of
HIV-1-positive cells to PLAP-positive cells declined from 1
on day 7 to
0.7 on day 14 but remained constant at this level
thereafter. We found
that 10% of cells were still positive for
HIV-1 antigens and 15% were
positive for PLAP 49 days after infection
(Fig.
5). Thus, within the
limits of this experiment, infected
astrocytes did not selectively
decrease the expression of structural
(late) HIV-1 proteins detected by
AIDS serum or upregulate the
expression of regulatory (early) viral
proteins, here indicated
by the surrogate marker PLAP. These results
confirm our earlier
data (Fig.
2 to
4) showing that a significant
proportion of HIV-1-infected
astrocytes continues to express structural
HIV-1 products for
several weeks after primary infection, indicating
that these cells
exhibit no intracellular restrictions to HIV-1
replication.

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[in this window]
[in a new window]
|
FIG. 5.
Expression of HIV-1 PLAP marker after pseudotyped HIV-1
infection. Astrocytes were infected with MLV/NL-P1 and evaluated at the
indicated times by IF staining with AIDS sera or anti-PLAP antibody as
described in Materials and Methods. Each time point represents counts
of 200 cells each in three different fields.
|
|
Astrocytes infected with pseudotyped HIV-1 produce infectious
virus.
To determine whether progeny virions made by astrocytes
infected with pseudotyped HIV-1 are infectious, supernatants were collected on days 14 and 21 after VSV/NL4-3 or MLV/NL4-3 infection of
astrocytes, standardized for p24 content, and were subjected to titer
determination for infectious HIV-1 by the MAGI assay (Fig.
6). Progeny virions collected at both
time points had 6 to 10 IU per 100 pg of p24 of culture supernatant
(Fig. 6). Thus, astrocytes producing HIV-1 can serve as a source of
infectious progeny virus.

View larger version (78K):
[in this window]
[in a new window]
|
FIG. 6.
HIV-1-infected astrocytes produce infectious progeny
virus. Astrocytes were infected with VSV/NL4-3 or MLV/NL4-3 as
described in the text, and culture supernatants were collected 14 and
21 days after infection, filtered through 0.45-µm-pore-size filters,
and tested for the presence of infectious virus in the MAGI assay.
Values represent means and standard deviations from three different
experiments.
|
|
 |
DISCUSSION |
Astrocytes are infected by HIV-1 in vivo (57, 67,
68), and it has been important to devise experimental systems to
investigate the course and consequences of their infection. Using HIV-1
capable of entry into such CD4-negative cells through pseudotyping with VSV or MLV envelope proteins, we have found that primary human fetal
astrocytes are permissive to highly productive HIV-1 infection. At the
peak of infection, up to 70% of astrocytes expressed HIV-1 antigens
and viral p24 production reached 1.7 µg/ml of culture supernatant
(Fig. 1 and 2). Virus expression then gradually declined, but 5 to 10%
of the cells still expressed virus antigens and secreted viral p24 at
0.1 µg/ml 7 weeks after infection, indicating persistent infection in
a substantial minority of cells. As observed in many previous studies
of astrocytes and other CD4-negative cells (7, 69),
infection by native NL4-3 was 3 orders of magnitude less productive
(Fig. 2). Similar to productively infected T cells (32),
pseudotyped HIV-1-infected astrocytes expressed the major HIV-1 RNA
species at equivalent levels, synthesized viral structural and
regulatory proteins, and released infectious progeny virions. We
conclude that the primary restriction to HIV-1 infection of astrocytes
is at virus entry and that once this block is surmounted, astrocytes
replicate HIV-1 efficiently for weeks before downregulating virus expression.
Transfection of viral DNA has been a method of choice to circumvent
inefficient HIV-1 entry into primary astrocytes. Using this method,
other investigators, as well as ourselves, have shown that astrocytes
can transiently express HIV-1 structural proteins (7, 21,
69). The results varied depending on the extent and period of
viral production, ranging from 5 to 20 days and from 200 to 50,000 pg
of viral p24 antigen per ml of culture medium (7, 69).
Different methods of transfection resulting in different levels of DNA
uptake may account for the ranges observed. Infection by pseudotyped
HIV-1 also results in transient viral expression; however, its period
is on the order of weeks and its extent is 1 to 2 orders of magnitude
higher than by transfection. The form of viral DNA introduced into
cells by these different approaches is likely to contribute to the
differences in the extent of viral expression. Transfected HIV-1 DNA is
embedded in plasmid DNA and lacks the viral proteins which mediate
nuclear entry and integration, and most of it is degraded in the
cytoplasm. In contrast, both VSV G protein and MLV envelope protein
mediate efficient uptake of retroviral nucleocapsid into cells,
initiating a conventional retroviral life cycle (2, 3,
64). Use of pseudotyped HIV-1 enabled us to investigate the
basic parameters of HIV-1 infection in astrocytes. We found that viral
doses comparable to a multiplicity of infection of 1 in T lymphocytes
i.e., about 1 pg of p24 per cell, when pseudotyped, were sufficient for
infection of 50 to 70% of astrocytes, indicating that after virus
entry, T lymphocytes and astrocytes are similarly susceptible to HIV-1
replication. The susceptibility of astrocytes to productive HIV-1
infection was highly reproducible. In multiple trials using different
virus stocks, cells from more than 20 donors secreted microgram levels of the structural protein p24 after infection by NL4-3 pseudotyped with
VSV or MLV envelope proteins. Consistent with p24 secretion, infected
astrocytes also produced infectious progeny virus, indicating that
HIV-1 can complete its life cycle in astrocytes, including all
posttranslational processing and assembly events. Indeed, rescue of
infectious HIV-1 from astrocytes was first reported in 1987 (13). These findings raise the possibility that astrocytes in the brain which carry HIV-1 may serve as a reservoir of infectious virus.
Using efficient infection, we revisited some of the basic questions
regarding HIV-1 replication in astrocytes. Given previous reports that
doubly spliced transcripts were preferentially expressed in astrocytes
following HIV-1 DNA transfection (69) and analogous findings of Nef but not envelope proteins in astrocytes from
HIV-1-infected brains (57), one goal of this work was to
investigate the relative expression of HIV-1 structural and regulatory
products by infected astrocytes. Northern blot analysis of viral RNA 1 week after pseudotype HIV-1 infection of astrocytes revealed expression
of the three major HIV-1 transcripts at similar levels; 2 or 3 weeks
after infection, the 9-kb genomic transcript was somewhat more abundant than the singly or doubly spliced transcripts, but all three were detectable by Northern blotting. To confirm that transcripts for structural and regulatory genes were similarly expressed, exported from
the nucleus, and translated by astrocytes in the present system, we
evaluated HIV-1 protein production by Western blotting and IF staining.
Env, Gag, and Nef were detectable by immunoblotting 1 week after
infection, and Gag was also detectable 5 weeks after infection,
consistent with the continued secretion of large amounts of p24 core
antigen. Similar findings were obtained using IF staining of the marker
protein, PLAP expressed from a doubly spliced mRNA like Nef (12,
18) or HIV-1 structural proteins. The numbers of cells
expressing structural proteins or PLAP were similar, reaching a peak of
about 30% of cells and declining at 7 weeks to 10 and 15%,
respectively. Our findings indicate that HIV-1 infection of primary
astrocytes results in a very high peak of coordinated expression of
viral structural and regulatory genes followed by a decline in parallel
of the major viral products over several weeks. Conversely, we have
seen no evidence in our system for preferential expression of the 2-kb
HIV-1 RNA and Nef protein observed in other systems (57,
69).
Another approach to investigate astrocyte susceptibility to HIV-1
infection in culture employed transformed astrocytic cell lines
transiently or stably transfected with HIV-1 DNA. Several studies found
specific and well-defined blocks to virus replication, including
abnormal HIV-1 RNA transcription (69), block of Rev function (42, 50), or inefficient translation of some
viral mRNA species (24). However, using different
glioblastoma cell lines, other investigators, including ourselves,
found that once appropriate receptors for virus entry were expressed,
the cells were highly susceptible to HIV-1 infection (61, 72,
74). In another study, we established chronically infected
U251-MG glioblastoma cell lines by transfection of HIV-1 DNA and drug selection (21). Like the system described here, these
cells also downregulated HIV-1 expression over time but with a
coordinated decline in viral products and no clear evidence of abnormal
HIV-1 RNA transcription or translation or of blockage of Rev function (59, 72). At this point it is not clear which of these
different styles of virus replication reflects the course of HIV-1
infection of astrocytes in the brain.
The consensus of many studies of brains from HIV-1-infected persons is
that astrocytes carry viral DNA at frequencies approximating 1%. It is
a very interesting question to ask what route of entry was used by
HIV-1 to establish infection in these CD4-negative cells, but the virus
seemed to be able to enter astrocytes and synthesize viral DNA. In
culture, transmission of HIV-1 to astrocytes by cell contact is more
efficient than exposure to cell-free virus (47), and this
may play a role in the brain. A different critical question is the
extent to which this HIV-1 DNA is expressed in astrocytes in the brain.
The consensus is that the majority of HIV-1-infected astrocytes do not
express viral RNA, at least at levels easily detected in productively
infected macrophages or microglia, although there are reports of HIV-1
RNA and structural proteins in astrocytes in the brain (25,
53). We suggest that the system described here is one reasonable
approach to investigate the regulation of viral DNA expression by
astrocytes. We have shown that cells initially synthesize the major
HIV-1 products, including infectious progeny virus, but that after a
time this expression is attenuated. Our system offers the possibility
of investigating the mechanism of this attenuation by ensuring that the
majority of astrocytes in culture are infected, express viral products,
and, later, coordinately downregulate this expression.
 |
ACKNOWLEDGMENTS |
We thank G. Benstman for technical assistance; H. Gendelman, L. Sharer, and G. Trillo-Pazos for their comments; and I. M. Totillo
for her help with the manuscript. We also gratefully acknowledge the
following colleagues for donation of reagents: M. Martin for the NL4-3
proviral clone, K. Collins for the NL-P1 clone, M. Emerman for the VSV
G vector, D. Littman for the MLV-envelope vector, B. Chesebro and H. Chen for hybridoma cells producing anti-p24 antibody, J. Laman for
anti-HIV-2 V3 antibody, and R. Swanstrom for anti-Nef antibody.
This work was supported by NIH grants to D.J.V., M.C., and M.J.P.
 |
FOOTNOTES |
*
Corresponding author. Mailing address: Division of
Molecular Virology, St. Luke's-Roosevelt Hospital Center, 432 West
58th St., Antenucci Research Bldg., Rm. 709, New York, NY 10019. Phone: (212) 582-4451. Fax: (212) 582-5027. E-mail:
djv4{at}columbia.edu.
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Journal of Virology, September 2001, p. 7925-7933, Vol. 75, No. 17
0022-538X/01/$04.00+0 DOI: 10.1128/JVI.75.17.7925-7933.2001
Copyright © 2001, American Society for Microbiology. All rights reserved.
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