Disrupted glial fibrillary acidic protein network in astrocytes from vimentin knockout mice

Glial fibrillary acidic protein (GFAP) is an intermediate filament protein expressed predominantly in astrocytes. The study of its expression in the astrocyte lineage during development and in reactive astrocytes has revealed an intricate relationship with the expression of vimentin, another intermediate filament protein widely expressed in embryonic development. these findings suggested that vimentin could be implicated in the organization of the GFAP network. To address this question, we have examined GFAP expression and network formation in the recently generated vimentin knockout (Vim-) mice. We show that the GFAP network is disrupted in astrocytes that normally coexpress vimentin and GFAP, e.g., those of the corpus callosum or the Bergmann glia of cerebellum. Furthermore, Western blot analysis of GFAP protein content in the cerebellum suggests that posttranslational mechanisms are implicated in the disturbance of GFAP network formation. The role of vimentin in this process was further suggested by transfection of Vim- cultured astrocytes with a vimentin cDNA, which resulted in the normal assembly of the GFAP network. Finally, we examined GFAP expression after stab wound-induced astrogliosis. We demonstrate that in Vim- mice, reactive astrocytes that normally express both GFAP and vimentin do not exhibit GFAP immunoreactivity, whereas those that normally express GFAP only retain GFAP immunoreactivity. Taken together, these results show that in astrocytes, where vimentin is normally expressed with GFAP fails to assemble into a filamentous network in the absence of vimentin. In these cells, therefore, vimentin appears necessary to stabilize GFAP filaments and consequently the network formation.     

Expression of vimentin and glial fibrillary acidic protein in human developing spinal cord

Summary Expression of intermediate filament proteins was studied in human developing spinal cord using immunoperoxidase and double-label immunofluorescence methods with monoclonal antibodies to vimentin and glial fibrillary acidic protein (GFAP). Vimentin was found in the processes of radial glial cells in 6-week embryos, while GFAP appeared in vimentin-positive astroglial cells at 8–10 weeks. GFAP and vimentin were present in approximately equal amounts in differentiating astrocytes in 23-week spinal cord. In 30-week fetuses, astrocytes reacted strongly for GFAP, while both the reaction intensity and the number of vimentin-positive cells fluctuated predominantly in the grey matter. No clear-cut transition from vimentin to GFAP was noticed during the development of astrocytes. The majority of ependymal cells in 23-week fetuses contained vimentin but only a few of them reacted for GFAP. The expression of vimentin continued during the whole development of the ependymal layer, in contrast to the reactivity for GFAP which disappeared between the 30th week and term.     

Effect of 6-hydroxydopamine (6-OHDA) on proliferation of glial cells in the rat cortex and striatum: evidence for de-differentiation of resident astrocytes

Reactive astrogliosis is the universal response to any brain insult. It is characterized by cellular hypertrophy, up-regulation of the astrocyte marker glial fibrillary acidic protein (GFAP), and proliferation. The source of these proliferating cells is under intense debate. Progenitor cells derived from the subventricular zone (SVZ), cells positive for chondroitin sulfate proteoglycan (NG2(+)), and de-differentiated astrocytes have been proposed as the origin of proliferating cells following injury. We have analyzed the effect of intraventricular-applied 6-hydroxydopamine (6-OHDA) on the proliferation and morphology of astrocytes in rat cortex and striatum by means of immunohistochemistry and confocal laser microscopy. At 4 days post-lesion, GFAP expression increased markedly. A subpopulation of the GFAP(+) cells co-expressed Ki-67, indicating that these cells were proliferating. To investigate whether these cells (1) arose from migrating SVZ progenitor cells, (2) derived from NG2(+) progenitor cells, or (3) de-differentiated from resident astrocytes, we studied the expression of the migration marker doublecortin (Dcx), the oligodendrocyte progenitor marker NG2, and the progenitor markers Nestin and Pax6. The proliferating Ki-67(+) cells co-expressed Nestin and Pax6, whereas no co-expression of Ki-67 with NG2 or the migration marker Dcx was observed. Thus, resident astrocytes de-differentiate, in response to the intraventricular application of 6-OHDA, to a phenotype resembling radial glia cells, which represent transient astrocyte precursors during development. An understanding of the mechanisms of the de-differentiation of mature astrocytes might be useful for designing new approaches to cell therapy in neurodegenerative diseases such as Parkinson's disease.     

A novel role of lactosylceramide in the regulation of tumor necrosis factor alpha-mediated proliferation of rat primary astrocytes. Implications for astrogliosis following neurotrauma

The present study describes the role of glycosphingolipids in neuroinflammatory disease and investigates tumor necrosis factor alpha (TNFalpha)-induced astrogliosis following spinal cord injury. Astrogliosis is the hallmark of neuroinflammation and is characterized by proliferation of astrocytes and increased glial fibrillary acidic protein (GFAP) gene expression. In primary astrocytes, TNFalpha stimulation increased the intracellular levels of lactosylceramide (LacCer) and induced GFAP expression and astrocyte proliferation. D-threo-1-phenyl-2-decanoylamino-3-morpholino-1-propanol.HCl (PDMP), a glucosylceramide synthase and LacCer synthase (GalT-2) inhibitor, inhibited astrocyte proliferation and GFAP expression, which were reversed by exogenous supplementation of LacCer but not by other glycosphingolipids. TNFalpha caused a rapid increase in the activity of GalT-2 and synthesis of LacCer. Silencing of GalT-2 gene using antisense oligonucleotides also attenuated the proliferation of astrocytes and GFAP expression. The PDMP and antisense-mediated inhibition of proliferation and GFAP expression was well correlated with decreased Ras/ERK1/2 pathway activation. Furthermore, TNFalpha-mediated astrocyte proliferation and GFAP expression was also inhibited by LY294002, a phosphatidylinositol 3-kinase inhibitor, which was reversed by exogenous LacCer. LY294002 also inhibited TNFalpha-induced GalT-2 activation and LacCer synthesis, suggesting a phosphatidylinositol 3-kinase-mediated regulation of GalT-2. In vivo, PDMP treatment attenuated chronic ERK1/2 activation and spinal cord injury (SCI)-induced astrocyte proliferation with improved functional recovery post-SCI. Therefore, the in vivo studies support the conclusions drawn from cell culture studies and provide evidence for the role of LacCer in TNFalpha-induced astrogliosis in a rat model of SCI. To our knowledge, this is the first report demonstrating the role of LacCer in the regulation of TNFalpha-induced proliferation and reactivity of primary astrocytes.     

Cytoskeletal Alterations in Human Fetal Astrocytes Induced by Interleukin-1β

Abstract: Previous studies in this and other laboratories have shown that interleukin-1β (IL-1β) is a selective and potent activator of human astrocytes with respect to induction of cytokines and hematopoietic growth factors. To study the effect of recombinant human IL-1β (rhIL-1β) on astrocyte morphology, glial fibrillary acidic protein (GFAP) and vimentin expression, and actin organization, we conducted a systematic survey using dissociated human fetal astrocyte cultures. Within hours of stimulation with IL-1β, the majority of astrocytes converted from flat, polygonal cells to small, contracted, highly branched cells. This change in morphology was more striking when serum was eliminated from the medium. Complete dissolution of filamentous actin occurred simultaneously with the change in cell shape, as demonstrated by fluorescein-phalloidin binding. These “activated” astrocytes displayed intense GFAP and vimentin immunoreactivity in the small perikarya and processes. In contrast, the large, flat astrocytes in control cultures showed diffuse pale immunoreactivity for GFAP and vimentin. To quantify the changes in GFAP and vimentin content with IL-1β stimulation, densitometric analyses of northern and western blots were performed. Northern blot analysis of IL-1β-stimulated astrocytes revealed a transient, marked decrease in steady-state levels of mRNA for GFAP, vimentin, and microtubule-associated protein 4. The decrease in mRNA levels was evident by 4–8 h and fell to the lowest level at 16–24 h (80–98% decrease by densitometry) with partial recovery by 72 h. By immunoblotting, a significant decrease in both GFAP and vimentin protein content was observed after IL-1β stimulation. Furthermore, metabolic labeling studies revealed an almost total loss of GFAP synthesis following stimulation with IL-1β for 16 h. These observations are consistent with the idea that increases in immunoreactivity were related to factors such as redistribution of epitope, rather than increases in total protein content. We hypothesize that in IL-1β-stimulated astrocytes, synthesis of other proteins, e.g., inflammatory cytokines, occurs at the expense of structural proteins and that the decrease in content of cytoskeletal proteins may reflect an “activated” state of astrocytes.     

Synthesis and Turnover of Cytoskeletal Proteins in Cultured Astrocytes

Abstract: We previously reported that the cytoskeleton of rat astrocytes in primary culture contains vimentin, glial fibrillary acidic protein (GFAP), and actin. These proteins were found in a fraction insoluble in Triton X-100 and thought to be assembled in filamentous structures. We now used primary astrocyte cultures to study the kinetics of synthesis and turnover of these cytoskeletal proteins. The intermediate filament proteins were among the most actively synthesized by astrocytes. High levels of synthesis were detectable by the third day of culture in the early log phase of growth, and the pattern of labeling at day 3 was similar to that at 14 days when the cultures had reached confluency. In short-term incorporation experiments vimentin, GFAP, and actin in the Triton-insoluble fraction were labeled within 5 min after exposure of the cultures to radioactive leucine. We did not detect any saturation of labeling for up to 6 h of incubation. The turnover of filament proteins studied by following the decay of radioactivity from prelabeled vimentin, GFAP, and cytoskeletal actin displayed biphasic decay kinetics for all three proteins. In the initial phase a fast-decaying pool with a half-life of 12–18 h contributed about 40% of the total activity in each protein. A major portion, about 60%, of each protein, however, decayed much more slowly, exhibiting a half-life of about 8 days.     

Glial shape and cytoskeletal protein synthesis

We investigated whether the shape of astroglial derived cells influences the expression of cytoskeletal proteins. In reaggregating cultures GFAP, vimentin and actin synthesis was approximately 52%, 50% and 37% the level found in monolayer cultures, respectively. Monolayer cultures consisted of polygonal shaped cells adhering to plastic, while reaggregating cultures were comprised of round cells growing in a suspension like culture. Additionally, human glioma cells induced to grow as round cells on poly-2-hydroxyethyl methacrylate (polyhema) coated plastic exhibited a level of GFAP synthesis that was approximately 20% the level displayed by polygonal shaped cells grown on uncoated plastic. Glioma cells initially grown on a polyhema surface and replated onto uncoated plastic were capable of reinitiating GFAP synthesis. Thus, aterations in the synthesis of GFAP and other cytoskeletal proteins can occur when astrocytes change their shape.     

Glial cells in the pineal gland of mice and rats

Summary Antigenic markers characteristic of astrocytes and their differentiative states (i.e., glial fibrillary acidic protein (GFAP), vimentin, and M1 and C1 antigens) were investigated in the pineal gland of mouse and rat using double immunolabeling techniques. In both species the socalled interstitial cells as characterized by TEM were shown to be astrocytes, since they expressed vimentin, but neither fibronectin (a marker for fibroblasts and endothelial cells) nor the neuron-specific L1 antigen or tetanus toxin receptors. Subpopulations of vimentin-positive pineal astrocytes were also GFAP- and C1- antigen-positive. M1- antigenpositive cells were not detected.It is concluded that a considerable proportion of interstitial cells in the pineal gland of rat and mouse are immature astrocytes which, in contrast to other parts of the central nervous system, persist into adulthood.Supported in part by Deutsche Forschungsgemeinschaft (Scha 185/9-4)S.-K. Huang was a recipient of a Humboldt Foundation fellowship.     

Growth Kinetics, Cell Shape, and the Cytoskeleton of Primary Astrocyte Cultures

Abstract: We examined correlations among growth kinetics, cell shape, and cytoskeletal protein content in rat astrocytes grown in primary culture. Cell suspensions from brains of newborn rats were seeded at densities from 0.2 to 3 × 10⁵/cm². At initial densities above 1 × 10⁵ the population increased to reach confluency by 10–12 days, after which cell number remained stable for many weeks. At low initial densities, 0.2–0.4 × 10⁵/cm², cells did not increase in number. Final density increased with increasing plating densities. High-density cells had small perikarya and several long cytoplasmic processes; low-density cells appeared flat and polygonal. All cultures were almost entirely astrocytic, as judged by immunofluorescent staining with antiserum against glial fibrillary acidic protein (GFAP). Cytoskeletal proteins were analyzed by gel electrophoresis after extraction from cells with nonionic detergent. Relative amounts of the proteins differed, in that low-density cells contained large amounts of cytoskeletal actin relative to the intermediate filament (IF) proteins vimentin and GFAP, whereas high-density cells contained relatively less actin and more IF proteins. Such differences in cytoskeletal proteins between the high- and low-density cultures were mirrored in the relative rates of synthesis of the cytoskeletal proteins. In the low-density cells amino acid incorporation into cytoskeletal-associated actin was more active than that into the IFs, whereas in the high-density cells higher rates of IF protein synthesis were observed.     

The intermediate filament complement of the retina: a comparison between different mammalian species

We compared the intermediate filament expression of the various cell types in the fully differentiated neural retina from rat, mouse, rabbit, guinea pig, cow, pig, and cat. Many cell types had an intermediate filament complement conserved across species boundaries, such as Müller cells and retinal ganglion cells. In some species (rabbit, guinea pig, and cow), however, we were unable to visualize GFA (glial fibrillary acidic)-positive retinal astrocytes, although such profiles were clearly visible in the remainder. Horizontal cell staining proved to be extremely species-variable. In rat and mouse the processes of these cells were identically displayed with antibodies to vimentin and all three neurofilament triplet proteins. In cow they decorated with antibodies to vimentin and antibodies to the two lower molecular weight neurofilament proteins alone, whereas in pig, rabbit and guinea pig all three neurofilament proteins but not vimentin were present. Finally cat horizontal cells stained for all three neurofilament proteins, some finer processes being additionally stainable with vimentin. A further surprise was the visualization of profiles positive only for the two lower molecular weight neurofilament proteins in the inner nuclear layer of both rabbit and guinea pig retina but not the other species. The implications of these results will be discussed.     

Spatiotemporal Gradient of Astrocyte Development in the Chick Optic Tectum: Evidence for Multiple Origins and Migratory Paths of Astrocytes

Astrocytes have been considered to be transformed from radial glial cells that appear at early stage of development and play a scaffold-role for neuronal cell migration. Recent studies indicate that neuroepithelial cells in the spinal cord also give rise to astrocytes. However, the mode of astroglial generation and migration in the ventricular neuroepithelium remains poorly understood. In this study, we have utilized immunohistochemical and retroviral lineage tracing methods to characterize the developmental profiles of astrocytes in the chick optic tectum, which develops from both the neural tube and invasion of optic tract. Chick vimentin and glial fibrillary acidic protein (GFAP) were found as single bands at molecular weights consistent with those reported for mammalian species. Differential developmental trends were observed for both proteins with relative vimentin levels decreasing and GFAP levels increasing with embryonic age. We observed two streams of tectal GFAP-labeled astrocytes originated from the tectal ventricle (intrinsic origin) and the optic tract (extrinsic origin). The extrinsic astrocytes arose from the ventral neuroepithelium of the third ventricle, dispersed bilaterally to the optic tract, and subsequently to the outer layer of optic tectum, indicating migration of astrocytes along retinal ganglion cell axons. On the other hand, the intrinsic astrocytes from the tectal ventricular neuroepithelium appeared first in the ventral part of the optic tectum, and then in the lateral and dorsal tectum. The intrinsic tectal astrocytes closely associated with fascicles of vimentin-labeled radial glial cells, indicating a presumptive radial migration of astrocytes. These results demonstrated that the optic tectum contains heterogeneous populations of astrocytes developed from the different origins and routes of migration.     

A comparison of the proliferative activity of astrocytes and astrocyte-like cells expressing vimentin in the injured mouse cerebral hemisphere.

After an unilateral injury of the cerebral hemisphere, 28 nice were injected with 3H thymidine at different intervals following the injury. Thereafter, the distribution of autographically labelled astrocytes expressing glial fibrillary protein (GFAP) and astrocyte-like cells expressing vimentin were recorded within the region of injury. Proliferative activity of the two cell types started at the same time, i.e. 24 h. after injury, reached its maximum on day 4, and returned to normal level after the 8th posttraumatic day. However, on day 4 the number of proliferating GFAP-positive astrocytes was about 50% higher than that of vimentin-positive cells. This was regarded as a proof of the concept that a significant number of astrocytes did not express vimentin during its mitotic cycle. Those facts were considered as an evidence against the hypothesis that a reactive astrocyte division induces a two-stage increase in the cytoskeletal proteins level with the elevated synthesis of vimentin preceding that of GFAP.     

The Cytoskeleton of Primary Astrocytes in Culture Contains Actin, Glial Fibrillary Acidic Protein, and the Fibroblast-Type Filament Protein, Vimentin

Abstract: Primary astrocytes were cultured from the forebrains of 1-day-old rats. Immunofluorescence microscopy showed that approximately 80% of the cells were positive for glial fibrillary acidic protein (GFAP) and >80% were stained with an antiserum to the molecular weight 58,000 fibroblast intermediate filament protein (vimentin). Gel electrophoresis of Triton-insoluble cytoskeleton preparations from these cultures revealed three major bands having molecular weights of 58,000, 51,000, and 42,000, together with some prominent lower-molecular-weight species. The protein of molecular weight 51,000 was not present in preparations from fibroblasts. Each of the three major astrocyte proteins was subjected to limited proteolysis, while two of the proteins were cleaved by cyanogen bromide. The electrophoretic peptide patterns of the 58,000 protein were similar to those of vimentin isolated from NIL-8 fibroblasts, and the patterns of the 51,000 protein were similar to those of GFAP isolated from rat spinal cord. The patterns of the protein of molecular weight 42,000 resembled those of muscle actin. Rocket immunoelectrophoresis showed that the 51,000 astrocyte protein reacted with an antiserum to bovine GFAP, but the 58,000 and 42,000 proteins failed to react. We conclude that the major proteins of cytoskeleton preparations from cultured primary astrocytes are vimentin (58,000), GFAP (51,000), and actin (42,000), and that our data show no obvious structural relationship among them.     

The Impact of Genetic Removal of GFAP and/or Vimentin on Glutamine Levels and Transport of Glucose and Ascorbate in Astrocytes

The importance of the intermediate filament (IF) proteins glial fibrillary acidic protein (GFAP) and vimentin for astrocyte function was studied by investigating astrocytes prepared from GFAP-/-and/or vimentin-/- mice. The rate of glucose uptake through facilitative hexose transporters was not affected by depletion of GFAP or vimentin. Similarly, the absence of these IF proteins did not affect ascorbate uptake, under control or cyclic AMP-stimulated conditions, or ascorbate efflux through volume-sensitive organic anion channels. However, compared with wild-type astrocytes, glutamine concentrations were increased up to 200% in GFAP-/- astrocytes and up to 150% in GFAP+/-astrocytes and this increase was not dependent on the presence of vimentin. GFAP-/- astrocytes in culture still contain IFs (made of vimentin and nestin), whereas GFAP-/-vim-/- cultured astrocytes lack IFs. Thus, glutamine levels appear to correlate inversely with GFAP, rather than depend on the presence of IFs per se. Furthermore, the effect of GFAP is dose-dependent since the glutamine concentration in GFAP+/- astrocytes falls between those in wild-type and GFAP-/-astrocytes.     

Electrophoretic pattern and distribution of cytoskeletal proteins in flat-epitheloid and stellate process-bearing astrocytes in primary culture

One- and two-dimensional electrophoresis patterns and distribution of major cytoskeletal proteins were studied in primary astrocytes with either flat-epitheloid or stellate appearance. No major differences in the electrophoretic patterns of actin, tubulin, glial fibrillary acidic protein (GFAP) and vimentin were detected between flat-epitheloid and stellate process-bearing astrocytes produced by the exposure of cultures to dibutyryl cyclic AMP (dBcAMP). However the morphological changes of astrocytes were accompanied by marked changes in the quantitative distribution of cytoskeletal proteins. The most prominent change was a large and specific decrease in the amount of actin, detected by [³⁵S]methionine incorporation, densitometric scanning of one-dimensional gels and DNase inhibition assay. In stellate astrocytes produced by a 4 day treatment with dibutyryl cyclic AMP, the amount of actin decreased by 50%. This decrease was not apparently related to the depolymerization of actin.     

P2Y nucleotide receptor interaction with alpha integrin mediates astrocyte migration

Astrocytes become activated in response to brain injury, as characterized by increased expression of glial fibrillary acidic protein (GFAP) and increased rates of cell migration and proliferation. Damage to brain cells causes the release of cytoplasmic nucleotides, such as ATP and uridine 5'-triphosphate (UTP), ligands for P2 nucleotide receptors. Results in this study with primary rat astrocytes indicate that activation of a G protein-coupled P2Y(2) receptor for ATP and UTP increases GFAP expression and both chemotactic and chemokinetic cell migration. UTP-induced astrocyte migration was inhibited by silencing of P2Y(2) nucleotide receptor (P2Y(2)R) expression with siRNA of P2Y(2)R (P2Y(2)R siRNA). UTP also increased the expression in astrocytes of alpha(V)beta(3/5) integrins that are known to interact directly with the P2Y(2)R to modulate its function. Anti-alpha(V) integrin antibodies prevented UTP-stimulated astrocyte migration, suggesting that P2Y(2)R/alpha(V) interactions mediate the activation of astrocytes by UTP. P2Y(2)R-mediated astrocyte migration required the activation of the phosphatidylinositol-3-kinase (PI3-K)/protein kinase B (Akt) and the mitogen-activated protein kinase/extracellular signal-regulated kinase (MEK/ERK) signaling pathways, responses that also were inhibited by anti-alpha(V) integrin antibody. These results suggest that P2Y(2)Rs and their associated signaling pathways may be important factors regulating astrogliosis in brain disorders.     

Development of cerebellar astroglia: Transitions in form and cytoskeletal content

The forms, disposition, and cytoskeletal contents of astroglia in immature mouse cerebellum were studied by immunocytochemical staining with antisera against two intermediate filament proteins, vimentin (Vim) (58,000 daltons) and glial filament protein (GF) (51,000 daltons). From embryonic (E) Day 15 to postnatal (P) Day 2, Vim is expressed in cells throughout the cerebellar anlage, including radial glia and Bergmann fibers, cells with amorphous shapes and 2–3 processes, and thick longitudinal elements oriented parallel to axons within axon tracts. GF is not expressed during the first few postnatal days, but by P7, there is a dramatic increase in GF-positive astrocyte-like cells in the putative white matter that are more densely stained and more crowded than at any other age. Between P7 and P14 all astrocytes throughout the cerebellum express both Vim and GF. From P21 on, Vim expression is progressively rarer in all astrocytes except for Bergmann fibers, and GF-positive astrocytes become less numerous. These findings raise two issues: (a) the lineage and relationships of cells expressing Vim and GF; (b) Since GF-positive cells appear as axon ingrowth ceases, axons must grow in a terrain comprised of glial cells that have a different cytoskeletal composition (vimentin), reflecting a less differentiated state, than mature astrocytes or than the GF-rich astrocytes that proliferate after injury in adult CNS.     

Role of Gap Junction Protein Connexin43 in Astrogliosis Induced by Brain Injury

Astrogliosis is a process that involves morphological and biochemical changes associated with astrocyte activation in response to cell damage in the brain. The upregulation of intermediate filament proteins including glial fibrillary acidic protein (GFAP), nestin and vimentin are often used as indicators for astrogliosis. Although connexin43 (Cx43), a channel protein widely expressed in adult astrocytes, exhibits enhanced immunoreactivity in the peri-lesion region, its role in astrogliosis is still unclear. Here, we correlated the temporal and spatial expression of Cx43 to the activation of astrocytes and microglia in response to an acute needle stab wound in vivo. We found large numbers of microglia devoid of Cx43 in the needle wound at 3 days post injury (dpi) while reactive astrocytes expressing Cx43 were present in the peripheral zone surrounding the injury site. A redistribution of Cx43 to the needle site, corresponding to the increased presence of GFAP-positive reactive astrocytes in the region, was only apparent from 6 dpi and sustained until at least 15 dpi. Interestingly, the extent of microglial activation and subsequent astrogliosis in the brain of Cx43 knockout mice was significantly larger than those of wild type, suggesting that Cx43 expression limits the degree of microgliosis. Although Cx43 is not essential for astrogliosis and microglial activation induced by a needle injury, our results demonstrate that Cx43 is a useful marker for injury induced astrogliosis due to its enhanced expression specifically within a small region of the lesion for an extended period. As a channel protein, Cx43 is a potential in vivo diagnostic tool of asymptomatic brain injury.     

Early Activation of STAT3 Regulates Reactive Astrogliosis Induced by Diverse Forms of Neurotoxicity

Astrogliosis, a cellular response characterized by astrocytic hypertrophy and accumulation of GFAP, is a hallmark of all types of central nervous system (CNS) injuries. Potential signaling mechanisms driving the conversion of astrocytes into “reactive” phenotypes differ with respect to the injury models employed and can be complicated by factors such as disruption of the blood-brain barrier (BBB). As denervation tools, neurotoxicants have the advantage of selective targeting of brain regions and cell types, often with sparing of the BBB. Previously, we found that neuroinflammation and activation of the JAK2-STAT3 pathway in astrocytes precedes up regulation of GFAP in the MPTP mouse model of dopaminergic neurotoxicity. Here we show that multiple mechanistically distinct mouse models of neurotoxicity (MPTP, AMP, METH, MDA, MDMA, KA, TMT) engender the same neuroinflammatory and STAT3 activation responses in specific regions of the brain targeted by each neurotoxicant. The STAT3 effects seen for TMT in the mouse could be generalized to the rat, demonstrating cross-species validity for STAT3 activation. Pharmacological antagonists of the neurotoxic effects blocked neuroinflammatory responses, pSTAT3^tyr705 and GFAP induction, indicating that damage to neuronal targets instigated astrogliosis. Selective deletion of STAT3 from astrocytes in STAT3 conditional knockout mice markedly attenuated MPTP-induced astrogliosis. Monitoring STAT3 translocation in GFAP-positive cells indicated that effects of MPTP, METH and KA on pSTAT3^tyr705 were localized to astrocytes. These findings strongly implicate the STAT3 pathway in astrocytes as a broadly triggered signaling pathway for astrogliosis. We also observed, however, that the acute neuroinflammatory response to the known inflammogen, LPS, can activate STAT3 in CNS tissue without inducing classical signs of astrogliosis. Thus, acute phase neuroinflammatory responses and neurotoxicity-induced astrogliosis both signal through STAT3 but appear to do so through different modules, perhaps localized to different cell types.     

Evolution of several cytoskeletal proteins of astrocytes in primary culture: Effect of prenatal alcohol exposure

In the present work we have analyzed, using immunoblotting and immunofluorescence techniques, the evolution of several cytoskeletal proteins during the development of astrocytes in primary culture. The effect of prenatal exposure to alcohol on these proteins was also evaluated. Microtubular protein -tubulin decreased approximately 47% from 4 to 7 days after which its content remained practically constant. Immunofluorescence studies showed also that the content of -tubulin was greater at day 4 of culture. This increase in fluorescence was coincident with the presence of globular particles which were found in interphase astrocytes and stained with both anti - and anti--tubulin. These structures appeared only in proliferating cells. Glial fibrillary acidic protein (GFAP) and vimentin were analyzed as intermediate filament (IF) proteins. GFAP, in cytoskeletal preparations, increased regularly for 14 days followed by a decrease to day 21. In contrast, vimentin showed a progressive increase throughout the entire culture period. Fluorescence studies revealed some differences between the IF distribution patterns of GFAP and vimentin.In astrocytes obtained from rats prenatally exposed to ethanol, decreases in the amounts of all the cytoskeletal proteins studied were found during the entire culture period. In these cells a striking disorganization of cytoskeleton was also observed. The alcohol-induced decrease of GFAP in cultured astrocytes was also found when this protein was studied in preparations from whole brain developed in vivo.Special issue dedicated to Dr. Santiago Grisolia