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PubMed1994

Differential changes in cell morphology, macromolecular composition and membrane protein profiles of neurons and astrocytes in chronic ethanol treated rats.

Cellular morphology, macromolecular composition, (DNA, RNA and Protein content) marker enzyme activities for neurons [neuron specific enolase (NSE)] and astrocytes [glutamine synthetase (GS)] and plasma membrane protein profiles in the bulk isolated neurons and astrocytes from control and ethanol treated rats were studied. One month aged Wistar rats were given ethanol as sole drinking fluid for 10 weeks. Scanning electron microscopy revealed a characteristic cell surface smoothening in astrocytes due to ethanol treatment. DNA levels were unaltered, while RNA and Protein contents were decreased in astrocytes and neurons. Further, 3H-leucine incorporation into proteins was decreased in neurons and astrocytes derived from ethanol treated rats indicating reduced protein synthesis in neurons and astrocytes. GS activity was affected severely suggesting impairment in astrocytic functions. Plasma membrane protein composition was analyzed by 2-D electrophoresis. The analysis indicated several protein defects in the plasma membranes of neurons and astrocytes, which might be involved in 'membrane disorder' during ethanol challenge. 125I-Wheat Germ agglutinin binding studies showed three prominent proteins (160, 116 and 97 kDa) in astrocyte membrane fraction suggesting the possible involvement of N-terminal glycoproteins in altered astrocyte morphology during ethanol ingestion. Impairment in the astrocyte cell functions, protein changes in plasma membrane and cellular morphology studies suggest that astrocytes may be more vulnerable than neurons for ethanol effects.

Alcoholism↗
PubMed1994

Abnormal astrocyte differentiation and defective cellular interactions in wobbler mouse spinal cord.

The wobbler mutation is inherited as an autosomal recessive trait and displays a muscular atrophy associated with motoneuron degeneration in early postnatal development. It has been shown that the level of glial fibrillary acidic protein (GFAP) is greatly increased in the spinal cord of wobbler mice. We performed immunocytochemical analyses combined with confocal microscopy to study the developmental distribution of GFAP-positive astrocytes in the spinal cord of wobbler mice during the course of the disease, and in primary cultures of adult wobbler spinal cord astrocytes. Many changes in the number and distribution of astrocytes were observed in the wobbler mice from 1-10 months post-partum. Strongly GFAP-positive astrocytes are present in small number in the anterior horn by 1 month. They increase in number and are observed in the entire spinal cord grey and white matters by 2-10 months. These reactive astrocytes have thick, short, extensively branched processes which contrast with the long, unbranched processes observed in control mice. The wobbler astrocyte processes are oriented perpendicular to the surface of the spinal cord, which contrasts with the normal parallel, concentric orientation. No expansion of astrocyte processes exit from the white matter towards the grey matter. Moreover, the surface of the wobbler spinal cord beneath the meninges displays a dramatic decrease of interdigitating processes, end feet and flattened cell bodies of astrocytes that form a disorganized layer. In vitro, mutant astrocytes have morphological characteristics similar to those in vivo and, in particular, develop short, thick, branched processes. These mutant astrocytes in cultures do not contact one another, whereas normal mature cultures show an increased incidence of cell-cell contacts between long processes. The increase of astrocyte reactivity associated with these modifications in astrocytic process arrangement may reflect an important primary event in the course of the wobbler disease rather than a non-specific response to motoneuronal death.

Animals↗
PubMed1992

Heterogeneous expression of carboxypeptidase E and proenkephalin mRNAs by cultured astrocytes.

Cultured astrocytes have been found to express neuropeptides, neuropeptide processing enzymes and their mRNAs. Although astrocytes were shown to display regional variation in their expression of these mRNAs, it was unclear whether all astrocytes cultured from the same brain region express similar mRNA levels or if this expression is heterogeneous. We examined the individual heterogeneity of astrocytes cultured from several brain regions by in situ hybridization. Astrocytes derived from the frontal cortex, hypothalamus and cerebellum of neonatal rat brains were cultured for 3 weeks and then analyzed by in situ hybridization using 35S-labeled cRNA probes to carboxypeptidase E (CPE), proenkephalin (PE), and cyclophilin (1B15) mRNAs and an oligomeric probe complimentary to the first 45 bases of rat 18S rRNA. Frequency histograms generated by counting the grains produced over emulsion-coated cells demonstrated populations of astrocytes expressing high levels of mRNA for CPE and PE and a population expressing low to background levels of these mRNAs. In contrast, all cultured astrocytes expressed high levels of 1B15 mRNA and 18S rRNA. The percentage of cultured astrocytes expressing high levels of CPE mRNA was 42% for frontal cortex astrocytes and 23% for cerebellar astrocytes. While the percentages of cultured astrocytes expressing high levels of PE mRNA varied slightly between brain region (24-28%), the level of PE mRNA expression per cell showed greater variation between regions. The effect of culture density on the expression of PE mRNA was also examined. Approximately 55% of the cells in low density cultures expressed PE mRNA, while only 5-10% of the cells in high density cultures expressed this mRNA. These results indicate that cultured astrocytes display individual heterogeneity with regard to neuropeptide biosynthesis and that the expression of neuropeptides by these cells is regulated.

Animals↗
PubMed1993

Endothelins modulate dibutyryl cAMP-induced stellation of cultured astrocytes.

Effect of endothelin-3 (ET-3) on dibutyryl cAMP (DBcAMP)-induced stellation of rat cerebral cultured astrocytes was examined. Treatment with 1 mM DBcAMP, 10 microM forskolin, 100 microM isoproterenol and 500 nM phorbol 12-myristate 13-acetate changed protoplasmic cultured astrocytes into process-bearing ones. ET-3 (1 nM) completely prevented the astrocytic stellation induced by these agents. The effect of ET-3 showed a dose-dependence, where IC50 value and maximal effective dose were 49 pM and about 0.1 nM, respectively. ET-1 and sarafotoxin (SRTX) S6b prevented the DBcAMP-induced astrocytic stellation with potencies similar to that of ET-3. ET-3 (1 nM) did not affect the cAMP accumulation after DBcAMP treatment in cultured astrocytes. Stellate astrocytes were reversed to the protoplasmic type cells by addition of 1 nM ET-3 in the presence of DBcAMP. ET-1 and SRTX similarly reversed the astrocytic stellation. ET-3 reversed the astrocytic stellation in the absence of extracellular Ca2+. Pre-loading of BAPTA-AM, a permeable Ca2+ chelator, on stellate astrocytes had no effect on the reversal by ET-3. ET-3 did not increase intracellular free Ca2+ concentration ([Ca2+]i) of most astrocytes tested at 0.1 nM. A high concentration (100 nM) of ET-3 increased astrocytic [Ca2+]i which was negated by Ca(2+)-free and BAPTA-AM loading. These results suggest that ETs modulate morphological changes in astrocytes through cAMP- and Ca(2+)-independent mechanisms.

Animals↗
PubMed1993

Opiates selectively increase intracellular calcium in developing type-1 astrocytes: role of calcium in morphine-induced morphologic differentiation.

Endogenous opioids and opiate drugs inhibit nervous system maturation, in part, by affecting the growth of astrocytes. Opiates inhibit astrocyte proliferation and cause premature differentiation. The emerging importance of Ca2+ in astrocyte function prompted us to explore whether opiates might affect astrocyte development by altering Ca2+ homeostasis. Astrocyte-enriched cultures were derived from newborn ICR mouse cerebra. Quantitative fluorescent measurements of intracellular free Ca2+ ([Ca2+]i) using Fura-2 as well as fluo-3 and computer-aided image analysis showed that 1 microM morphine significantly increased [Ca2+]i in flat, polyhedral, glial fibrillary acidic protein (GFAP) immunoreactive astrocytes at 2 and 6 min, and at 72 h. Co-administration of 3 microM naloxone blocked morphine-dependent increases in [Ca2+]i. Treatment with 1 microM concentrations of the kappa-opioid receptor agonist, U69,593, but not equimolar amounts of mu ([D-Ala2,MePhe4,Gly(ol)5]enkephalin)- or delta ([D-Pen2,D-Pen5]enkephalin)-opioid receptor agonists, significantly increased [Ca2+]i in astrocytes. To assess the role of Ca2+ in morphine-induced astrocyte differentiation, untreated and 1 microM morphine-treated astrocyte cultures were incubated for 5 days in < 0.01, 0.3, 1.0, or 3.0 mM extracellular Ca2+ ([Ca2+]o), or incubated with 1.0 mM [Ca2+]o in the presence of 1 microM of the Ca2+ ionophore, A23187. The areas of single astrocytes were measured and there was a positive correlation between astrocyte area and [Ca2+]o. Morphine had an additive effect on area and form factor measures when [Ca2+]o was 1.0 mM. High [Ca2+]o (3.0 mM) alone mimicked the action of morphine. Morphine alone had no effect on astrocyte area in the presence of 3.0 mM Ca2+.(ABSTRACT TRUNCATED AT 250 WORDS)

Animals↗
PubMedDate not supplied

Astrocytic contributions to blood-brain barrier (BBB) formation by endothelial cells: a possible use of aortic endothelial cell for in vitro BBB model.

Astrocytic contribution of endothelial cell monolayer permeability was examined in two blood-brain barrier (BBB) models, using the coculture in a double chamber system: rat astrocytes and bovine aortic endothelial cells (BAECs) or bovine brain endothelial cells (BBECs). In system 1, where astrocytes were separated from endothelial cells, a 40% reduction in L-glucose permeability of the BBEC monolayer, but not the BAEC monolayer, was observed by cocultivation with astrocytes. Although several passages of BBEC in culture elicited morphological transformation from spindle-shapes to cobblestone-like features, the passaged BBECs remained responsive to astrocytes in coculture in system 1 (37% reduction of the L-glucose permeability). By contrast, in system 2, where respective endothelial cells and astrocytes layered on the upper and lower surfaces of a membrane, the permeability of both BAEC and BBEC monolayers was reduced by cocultivation with astrocytes (75% reduction for BAEC and 40% reduction for BBEC). BAECs in this contiguous coculture (system 2) with astrocytes showed numerous tight junction-like structures characteristic of the BBB in vivo. These results suggest that primary cultured BBECs, which had been primed by astrocytes in vivo, retain a higher sensitivity to astrocytes possibly through an astrocytic soluble factor (s) to exhibit BBB-specific phenotypes, and that even BAEC from extra-neural tissues, when cultured with astrocytes in close proximity in vitro, may acquire the similar phenotypes and serve for an extensive use of BBB model in vitro.

Animals↗
PubMed1990

Growth of canine distemper virus in cultured astrocytes: relationship to in vivo persistence and disease.

Canine distemper virus (CDV) causes an encephalomyelitis in dogs which varies with the viral strain. The CDV Cornell A75-17 strain produces a delayed, subacute to chronic, demyelinating CNS disease. In contrast, the Snyder Hill (CDV-SH) strain-associated neurological disease is more acute in onset, is usually non-demyelinating and primarily produces lesions in the gray matter. In these studies we describe the effects of these two virulent and one avirulent CDV strain, Rockborn (CDV-RO), on astrocytes in dissociated canine brain cell cultures. In multiple replicate experiments, astrocytes were infected most rapidly by CDV-RO [100% of astrocytes were infected by 14 days post-inoculation (p.i.)]. This strain caused severe cytopathic effect (CPE) and cytolysis. CDV-SH similarly produced a rapid infection of the astrocytes. In contrast, CDV A75-17 infected less than 25% of the astrocyte population during the first 28 days p.i. (+/- 7 days); after 28 days p.i., a rapid rise in astrocyte infection occurred. Both virulent viruses caused astrocytic syncytial formation but did not cause cytolysis of the astrocyte population as was observed with the attenuated virus. Titers of infectious virus, released into the supernatant fluid, reflected the degree of astrocyte infection. Virus released by the cultures late in CDV A75-17 infection showed enhanced ability to infect newly derived astrocytes; in contrast, brain cell passaged CDV-SH did not show increased growth in these cells. These results show that (1) there is a difference in growth rate, CPE and capacity for adaptation of three different CDV strains in astrocytes in vitro, and (2) some aspects of the disease (such as persistence in white matter) produced by the virulent strains in vivo may be related to the course of astrocyte infection observed in vitro.

Animals↗
PubMed2005

Co-culture of neurones with glutathione deficient astrocytes leads to increased neuronal susceptibility to nitric oxide and increased glutamate-cysteine ligase activity.

The antioxidant glutathione (GSH) plays an important role in protecting the mitochondrial electron transport chain (ETC) from damage by oxidative stress in astrocytes and neurones. Neurones co-cultured with astrocytes have greater GSH levels, compared to neurones cultured alone, leading to the hypothesis that astrocytes play a key role in brain GSH metabolism by supplying essential GSH precursors to neurones. A previous study has postulated that damage to the ETC following exposure to reactive nitrogen species (RNS) is less in co-cultured neurones, compared to neurones cultured alone, because of the greater GSH levels in the former cells. To investigate this further, primary culture rat neurones were co-cultured with either rat astrocytes activated with IFN-gamma and LPS to produce NO, or NO-generating astrocytes that had been depleted of intracellular GSH by 87% following incubation with the GSH synthesis inhibitor L-buthionine-S,R-sulfoximine (L-BSO). Neurones incubated with NO-generating astrocytes depleted of GSH were unable to elevate GSH levels, unlike neurones co-cultured with NO-generating astrocytes. Complexes II + III and IV of the neuronal ETC were significantly inhibited following exposure to NO-generating astrocytes depleted of GSH. No ETC damage was observed in neurones co-cultured with NO-generating astrocytes. Although neurones co-cultured with GSH depleted astrocytes did not increase cellular GSH levels, the activity of glutamate cysteine ligase (GCL), the rate-limiting enzyme of GSH synthesis, was increased by 218%, compared to neurones cultured with control astrocytes. This suggests that neuronal GCL activity could be modulated when GSH metabolism is inhibited in neighboring astrocytes.

Animals↗
PubMed2006

Protection of ischemic brain cells is dependent on astrocyte-derived growth factors and their receptors.

An in vitro ischemia model (oxygen, glucose, and serum deprivation) is used to investigate the possible cellular and molecular mechanisms responsible for cerebral ischemia. We have previously demonstrated that supernatants derived from ischemic microglia can protect ischemic brain cells by releasing GDNF and TGF-beta1. In the present study, we investigate whether products of ischemic astrocytes can also protect ischemic microglia, astrocytes, and neurons in a similar manner. Supernatants from ischemic astrocytes were collected after various periods of ischemia and incubated with microglia, astrocytes, or neurons individually, under in vitro ischemic conditions. The components responsible for the protective effects of astrocyte-derived supernatants were then identified by Western blot, ELISA, trypan blue dye exclusion, and immunoblocking assays. Results showed that under conditions of in vitro ischemia the number of surviving microglia, astrocytes, and neurons was significantly increased by the incorporation of the astrocyte-derived supernatants. Astrocyte supernatant-mediated protection of ischemic microglia was dependent on TGF-beta1 and NT-3, ischemic astrocytes were protected by GDNF, and ischemic neurons were protected by NT-3. In addition, protein expression of TGF-beta1 and NT-3 receptors in microglia, GDNF receptors in astrocytes, and NT-3 receptors in neurons was increased by in vitro ischemia. These results suggest that astrocyte-derived protection of ischemic brain cells is dependent not only on factors released from the ischemic astrocytes, but also on the type of receptor present on the responding cells. Therapeutic potential of TGF-beta1, GDNF, and NT-3 in the control of cerebral ischemia is further suggested.

Animals↗
PubMed2005

Ca2+ signaling, mitochondria and sensitivity to oxidative stress in aging astrocytes.

Age-related changes in astrocytes that could potentially affect neuroprotection have been largely unexplored. To test whether astrocyte function was diminished during the aging process, we examined cell growth, Ca2+ signaling, mitochondrial membrane potential (DeltaPsi) and neuroprotection of NGF-differentiated PC12 cells. We observed that cell growth was significantly slower for astrocytes cultured from old (26-29 months) mice as compared to young (4-6 months) mice. DeltaPsis in old astrocytes were also more depolarized (lower) than in young astrocytes and old astrocytes showed greater sensitivity to the oxidant tert-butyl hydrogen peroxide (t-BuOOH). ATP-induced Ca2+ responses in old astrocytes were consistently larger in amplitude and more frequently oscillatory than in young astrocytes, which may be attributable to lower mitochondrial Ca2+ sequestration. Finally, NGF-differentiated PC12 cells that were co-cultured with old astrocytes were significantly more sensitive to t-BuOOH treatment than co-cultures of NGF-differentiated PC12 cells with young astrocytes. Together, these data demonstrate that astrocyte physiology is significantly altered during the aging process and that the astrocyte's ability to protect neurons is compromised.

Aging↗
PubMed2001

Activated astrocytes with glycogen accumulation in ischemic penumbra during the early stage of brain infarction: immunohistochemical and electron microscopic studies.

Brain infarction was induced in rats by injection of microspheres through the right internal carotid artery, and structural changes in the astrocytes were observed during the early period following the infarction. Necrotic foci, varying in size and shape, were found in the right hemisphere. After immunohistochemical staining for GFAP, GFAP-positive astrocytes in the perinecrotic area known as the ischemic penumbra had distinctly increased in number and size with elongation of cytoplasmic processes 3 days after infarction. Electron microscopic observation revealed that glycogen granules had markedly accumulated in the cytoplasm of astrocytes located in the ischemic penumbra 3 and 5 days after infarction. Seven days after infarction, however, the glycogen granules disappeared from the astrocytes. Intermediate filaments increasingly appeared in the protoplasmic astrocytes after 3 days and were abundant in the activated and hypertrophied astrocytes after 7 days. As a result of our present study, we conclude that: (1) the function of glucose uptake from blood vessels was not impaired in the astrocytes under hypoxic conditions; (2) the astrocytes actively ingested blood glucose through the endothelial cells and accumulated it as glycogen for activation of their functions, and the cell volume increased under hypoxic conditions; (3) the depression of energy metabolism and the decrease in the uptake of energy sources in the nerve cells promoted glycogen accumulation in the astrocytes under hypoxic conditions; (4) intermediate filaments (GFAP filaments) increased in number, coincident with the activation and enlargement of the astrocytes; and (5) protoplasmic astrocytes were transformed into fibrous astrocytes in the ischemic penumbra of the brain infarction.

Animals↗
PubMed1996

Rubral astrocytic reactions to proximal and distal axotomy of rubrospinal neurons in the rat.

Spinal tractotomy-induced perineuronal astrocytic reaction of the rat rubrospinal system was studied using an antiserum to the astrocyte-specific glial fibrillary acidic protein as a marker. The effect of the proximity of axonal cut to cell bodies was also studied by comparing astrocytic reactions elicited by upper cervical and lower thoracic tractotomy. Fast blue was used as a retrograde tracer to identify axotomized neurons, which were found to concentrate in the caudal part of the contralateral red nucleus. The length of reactive astrocytic processes in the dorsomedial and ventrolateral parts of the nucleus was quantified separately since neurons in these two parts project to cervical and lumbar spinal cord, respectively. Those of the ipsilateral nucleus were also quantified. Sham operation caused a transient increase in reactive astrocytic processes one day after surgery. An early and a late increase of reactive astrocytic processes was found 2-5 days and 2-8 weeks following both thoracic and cervical tractotomy. Cervical axotomy of lumbar-cord-projecting rubral neurons caused an increase of reactive astrocytic processes similar in magnitude to that generated by thoracic axotomy. Following thoracic axotomy, the uninjured dorsomedial area of the contralateral nucleus also displayed an increase concomitant with that which occurred within the neighboring, injured ventrolateral nuclear area suggesting the action of diffusible factor(s). Surprisingly, cervical and thoracic tractotomy also elicited a similar increase of reactive astrocytic processes in the ipsilateral nuclei, independent of the number of ipsilaterally projected neurons present in each nucleus. This may be attributed to the retrograde influence from the denervated spinal target sites which were carried by fibers of the intact rubrospinal tract known to terminate bilaterally. In the lesioned nucleus, reactive astrocytic processes were often located close to axotomized cell bodies as early as 3 days following upper cervical and also, to a lesser extent, lower thoracic tractotomy. However, reactive astrocytic processes in the ipsilateral nucleus usually remained in the neuropil. These results suggest that axotomy induces two levels of retrograde astrocytic reactions within the soma area of intrinsic central neurons. Reactive astrocytic processes located proximally to axotomized cell bodies may have a different functional role from those distributed in the neuropil.

Animals↗
PubMed1998

Induction of astrocyte metallothioneins (MTs) by zinc confers resistance against the acute cytotoxic effects of methylmercury on cell swelling, Na+ uptake, and K+ release.

Metallothionein (MT) proteins play an important role in the detoxification of heavy metals. Since methylmercury (MeHg) preferentially accumulates in astrocytes, we investigated the ability of the astrocyte-specific MT isoform, MT-I, to attenuate MeHg-induced cytotoxicity. Increased astrocytic MT expression was achieved by 24-h pretreatment of neonatal rat primary astrocyte cultures with 100 microM zinc (ZnSO4). Subsequently, the astrocytes were treated with MeHg (10 microM), and its toxic effects on cell volume, Na+ uptake, and K+ release were investigated and compared to cells treated with or without MeHg, but in the absence of Zn pretreatment. Pretreatment of astrocytes with Zn was associated with a 2.9-fold increase in MT protein levels (P<0.02), and a 5.6-fold increase in MT mRNA levels (p<0.002) compared to control astrocytes. Astrocytes expressing increased MT protein levels were resistant to MeHg-induced swelling. In isotonic buffer the effect of MeHg on swelling was abolished (p<0.01) by 24-h Zn pretreatment, in such a way that volume profiles in these cells did not differ from controls. Zn-induced increased expression of MTs was also associated with significant attenuation of astrocytic Na+ uptake (p<0.01) and Rb+ (a marker for K+) release (p<0.001) in response to treatment with MeHg. These results demonstrate (1) that astrocytes can be induced to express high levels of MT proteins by pretreatment with Zn, and (2) that Zn confers resistance against the acute effect of MeHg on astrocytic swelling and the associated changes in ion (Na+ and K+) transport. Taken together, the data suggest that astrocytic MT induction offers effective cellular adaptation to MeHg cytotoxicity.

Animals↗
PubMed2000

Multi-lipofection efficiently transfected genes into astrocytes in primary culture.

This study demonstrated that liposome-mediated transfection - lipofection - is suitable for delivering genes into astrocytes. By repeatedly lipofecting the same astrocyte cultures, a process we call multi-lipofection, the transfection efficiency of the beta-galactosidase (beta-gal) gene was improved from 2.6+/-0.6 to 17. 4+/-1.1%. This is the highest efficiency ever reported in gene-transfer with Lipofectin(R) in a primary culture of mouse cerebral cortical astrocytes. Furthermore, multi-lipofection did not cause observable disturbance to astrocytes as indicated by insignificant changes in the glial fibrillary acidic protein content in the cultures. In order to demonstrate that the transfected gene achieved a physiologically relevant expression level, a plasmid containing the pEF-hsp70 protein gene was lipofected into astrocytes. This produced colonies of astrocytes showing an increased resistance to heat-induced cell death. A similar experiment was performed with the glial-derived neurotrophic factor (GDNF) gene. Control astrocytes had no detectable GDNF. In the transfected astrocytes, the GDNF protein could be identified intracellularly by immunocytochemistry. Western blot analysis revealed, as compared to astrocytes with one lipofection, a 2.9-fold increase of GDNF with four lipofections. GDNF remained detectable in astrocytes 2 weeks after four lipofections. Thus, multi-lipofection provides a mild and efficient means of delivering foreign genes into astrocytes in a primary culture, making astrocytes good candidate vehicle cells for gene/cell therapy in the CNS.

Animals↗
PubMed1999

Tissue oxygen levels control astrocyte movement and differentiation in developing retina.

Astrocytes play a key role in the development of retinal vessels by detecting hypoxia in developing retina and secreting the hypoxia-induced angiogenic factor VEGF to induce vessel formation. The astrocytes which play this role are themselves spreading over the retina, just ahead of the growing vessels. To understand the mechanisms which keep astrocytes in this strategic 'just ahead' position we have studied the effects of hyperoxia and hypoxia on astrocyte differentiation and movement in situ in neonatal rat retina and in primary culture. Hyperoxia in situ inhibited the stellation of astrocytes, so that they persisted in a relatively unbranched form, which accumulated at the edge of their spreading population; hyperoxia permitted but did not accelerate migration. Conversely, hypoxia induced unstellated astrocytes to stellate within 6 h. If the hypoxia was abnormally severe, it caused the astrocytes to hyperstellate and slowed their spread. Astrocytes in primary culture did not change morphology or motility when challenged by hypoxia. When treated with medium conditioned by retina however, astrocytes became mobile and, if the medium was conditioned by hypoxic retina, became stellate. These results suggest that the oxygen released by retinal vessels maintains the mobility of astrocytes, via a diffusible factor released by other retinal cells. Conversely, naturally generated hypoxia of developing retina plays a triple role, inducing astrocytes to stellate, to end their migration and to produce VEGF, thereby inducing vessel formation. The induction of stellation is mediated by a diffusible factor released by other retinal cells. Thus hypoxia of the retina generated by neural maturation induces key events in both the differentiation of astrocytes and the formation of blood vessels.

Aging↗
PubMed1998

Altered taurine release following hypotonic stress in astrocytes from mice deficient for GFAP and vimentin.

Astrocytes maintain their volume in response to changes in osmotic pressure in their environment by an afflux/influx of ions and organic osmoequivalents. The initial swelling of an astrocyte transferred to a hypoosmotic medium is thus reversed within minutes. The mechanisms which trigger this process as well as the sensors for cell volume are largely unknown, however, the cytoskeleton appears to be involved. We have addressed the role of one component of the cytoskeleton, the intermediate filaments, in the maintenance of astrocytic cell volume. Astrocytes from wild type mice were compared with cells from mice deficient for either glial fibrillary acidic protein (GFAP-/-) or vimentin (vimentin-/-) and with astrocytes from mice deficient for both proteins (GFAP-/-vim-/-). Whereas GFAP-/- and vimentin-/- cultured or reactive astrocytes retain intermediate filaments, the GFAP-/-vim-/- astrocytes are completely devoid of these structures. The rate of efflux of the preloaded osmoequivalent 3H-taurine from primary and passaged cultures of astrocytes was monitored. A reduction of NaCl (25 mM) in the perfusion medium led to a 400-900% increase of 3H-taurine afflux in astrocytes from wild type mice. The stimulated efflux was not significantly affected in astrocytes from GFAP-/- or vimentin-/- mice. However, the efflux from astrocytes from GFAP-/-vim-/- mice was 25-46% lower than the wild type levels. The results strengthen the role of the cytoskeleton in astrocyte volume regulation and suggest an involvement of intermediate filaments in the process.

Animals↗
PubMed1998

Astrocytes are more vulnerable than neurons to cellular Ca2+ overload induced by a mitochondrial toxin, 3-nitropropionic acid.

The differential effects of 3-nitropropionic acid on cultured neurons and astrocytes (of cortical and striatal origin) were examined by studying intracellular Ca2+ changes using imaging techniques with fura-2. The neurons and astrocytes whose intracellular Ca2+ concentration was recorded were identified later by immunocytochemical staining for microtubule-associated protein 2 and glial fibrillary acidic protein, respectively. 3-Nitropropionic acid (1.7 mM) irreversibly increased intracellular Ca2+ in astrocytes (27%) and, to a significantly smaller extent, in neurons (10%). The latency to onset of the intracellular Ca2+ increase was longer in neurons (45 min) than in astrocytes (29 min). Thus, a differential susceptibility of astrocytes and neurons was observed. The 3-nitropropionic acid-induced astrocytic and neuronal Ca2+ accumulations were both due to influx of Ca2+, as the increases were absent in Ca2+-free medium. An inhibitor of the Na+-Ca2+ exchanger (2',4'-dichlorobenzamil), greatly reduced the intracellular Ca2+ increase in astrocytes, but not in neurons. This indicates that the intracellular Ca2+ increase in astrocytes is primarily mediated by a reverse operation of the Na+-Ca2+ exchange system, whereas in neurons it is mediated by a different mechanism. In addition, we noted that astrocytic cell death occurred in 9% of cells at 60 min or more after the start of a 40 min perfusion with 3-nitropropionic acid, while only 4% of neurons died. In astrocytes, cell death was preceded by blebbing of the cell membrane, and by a sustained increase in intracellular Ca2+ followed by an abrupt further elevation occurring just before cellular collapse. The present results indicate that astrocytes are more vulnerable than neurons to 3-nitropropionic acid-induced cellular Ca2+ overload and toxicity, and hence support the hypothesis that, in part, 3-nitropropionic acid-induced neurotoxicity could be secondary to astrocytic cell death caused by Ca2+ overload.

Amiloride↗
PubMed2006

Energy metabolism in astrocytes: high rate of oxidative metabolism and spatiotemporal dependence on glycolysis/glycogenolysis.

Astrocytic energy demand is stimulated by K(+) and glutamate uptake, signaling processes, responses to neurotransmitters, Ca(2+) fluxes, and filopodial motility. Astrocytes derive energy from glycolytic and oxidative pathways, but respiration, with its high-energy yield, provides most adenosine 5' triphosphate (ATP). The proportion of cortical oxidative metabolism attributed to astrocytes ( approximately 30%) in in vivo nuclear magnetic resonance (NMR) spectroscopic and autoradiographic studies corresponds to their volume fraction, indicating similar oxidation rates in astrocytes and neurons. Astrocyte-selective expression of pyruvate carboxylase (PC) enables synthesis of glutamate from glucose, accounting for two-thirds of astrocytic glucose degradation via combined pyruvate carboxylation and dehydrogenation. Together, glutamate synthesis and oxidation, including neurotransmitter turnover, generate almost as much energy as direct glucose oxidation. Glycolysis and glycogenolysis are essential for astrocytic responses to increasing energy demand because astrocytic filopodial and lamellipodial extensions, which account for 80% of their surface area, are too narrow to accommodate mitochondria; these processes depend on glycolysis, glycogenolysis, and probably diffusion of ATP and phosphocreatine formed via mitochondrial metabolism to satisfy their energy demands. High glycogen turnover in astrocytic processes may stimulate glucose demand and lactate production because less ATP is generated when glucose is metabolized via glycogen, thereby contributing to the decreased oxygen to glucose utilization ratio during brain activation. Generated lactate can spread from activated astrocytes via low-affinity monocarboxylate transporters and gap junctions, but its subsequent fate is unknown. Astrocytic metabolic compartmentation arises from their complex ultrastructure; astrocytes have high oxidative rates plus dependence on glycolysis and glycogenolysis, and their energetics is underestimated if based solely on glutamate cycling.

Animals↗