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C-terminal tail of beta-adrenergic receptors: immunocytochemical localization within astrocytes and their relation to catecholaminergic neurons in N. tractus solitarii and area postrema.

beta-Adrenergic receptors (beta AR) in the medial nuclei of tractus solitarii (m-NTS) and area postrema (AP) may bind to catecholamines released from neurons, whereas only the AP has fenestrated capillaries allowing access to circulating catecholamines. Since varied autonomic responses are seen following beta AR activation of the dorsal vagal complex, including the m-NTS and AP, we hypothesized that there might be a cellular basis for varied responses to beta AR stimulation that depends on the differential access to circulating catecholamines. Therefore, we comparatively examined the ultrastructural localization of the beta AR in relation to catecholaminergic neurons in these regions. An antibody directed against the C-terminal tail (amino acids 404-418) of hamster beta-adrenergic receptor (beta AR404) was used in this study. The localization of beta AR404 was achieved by the avidin-biotin peroxidase complex (ABC) technique in combination with a pre-embed immunogold labeling method to localize tyrosine hydroxylase (TH), the catecholamine-synthesizing enzyme. Within m-NTS and at subpostremal border, labeling for beta AR404 was evident along the intracellular surface of plasma membranes of small, apparently distal, astrocytic processes. Astrocytic processes with beta AR404-immunoreactivity formed multiple, thin lamellae around TH-labeled and non-TH neuronal cell bodies and dendrites. beta AR404-immunoreactive astrocytes also extended end-feet around blood vessels and surrounded groups of axon terminals that were directly juxtaposed to each other. Some, but not all, of these axons demonstrated TH-immunoreactivity. Fewer beta AR404-immunoreactive astrocytes were detected in AP, regardless of their proximity to catecholaminergic processes or blood vessels. The present astrocytic localization of beta AR404, together with the earlier, neuronal localization of beta AR's third intracellular loop, suggest that the beta AR may be substantially different between neurons and astrocytes. The regional difference in the prevalence of beta AR404-immunoreactive astrocytes suggests that these receptive sites may either: (i) be preferentially activated by catecholamines released from terminals rather than circulating catecholamines; or (ii) be down-regulated in AP due to blood-born substances, such as catecholamines. The extensive localization of beta AR in the border between m-NTS and AP also suggests that catecholaminergic activation of these astrocytes may dictate the degree of diffusion of catecholamines which are of neuronal or vascular origin. The specific localization of beta AR404-immunoreactivity to the more distal portions of astrocytes suggests the possibility that astrocytes have restrictive distributions of beta AR and that the beta-adrenergic activation lead to morphological or chemical changes that are also localized to the distal portions of astrocytes.(ABSTRACT TRUNCATED AT 400 WORDS)

Animals↗

Cultured astrocytes express mRNA for peptidylglycine-alpha-amidating monooxygenase, a neuropeptide processing enzyme.

Cultured astrocytes have been previously found to express several neuropeptides, as well as the neuropeptide processing enzyme carboxypeptidase E (CPE). To investigate whether cultured astrocytes contain additional peptide-processing enzymes, Northern blots were screened for peptidylglycine-alpha-amidating monooxygenase (PAM) mRNA. PAM is involved with the formation of amide groups on the C-terminus of numerous peptide hormones and neurotransmitters. Primary cultures of astrocytes contain moderate levels of PAM mRNA, as determined by Northern blot analysis. The level of PAM mRNA in cultured hypothalamic astrocytes is similar to the level expressed in cultured hypothalamic neurons. The relative abundance of PAM mRNA differs up to 6-fold between astrocytes cultured from various brain regions. Astrocytes cultured from hypothalamus have high levels of PAM mRNA, those cultured from striatum, frontal cortex, and hippocampus have moderate levels, and those cultured from cerebellum have low levels. To investigate whether all cultured astrocytes express PAM mRNA, in situ hybridization analysis of cultured astrocytes was performed. Interestingly, virtually all of the astrocytes cultured from either hypothalamus or cerebellum express PAM mRNA, in contrast to a previous finding that only 20-40% of similarly cultured astrocytes express CPE. The presence of PAM mRNA in cultured astrocytes suggests that these cells have the capacity to produce amidated neuropeptides.

Animals↗

Immunocytochemical and ultrastructural characterization of type 1 astrocytes and 0-2A lineage cells in long-term co-cultures.

We examined cultures of purified type 1 astrocytes and mixed glial co-cultures containing type 1 astrocytes and 0-2A lineage cells in media containing fetal calf serum at 5 days in vitro (DIV), 12 DIV, and 30 DIV, using cell-specific immunocytochemical markers and electron microscopy. At all three time points and in both culture systems, the polygonal-shaped type 1 astrocytes were A2B5-, GFAP+, and GalC-(specific markers for 0-2A lineage cells, and mature astrocytes and oligodendrocytes, respectively). From 5 to 30 DIV, the type 1 astrocytes increased markedly in size and the appearance of the cytoskeleton changed dramatically, with the amount of glial filaments increasing and microtubules decreasing. At 5, 12, and 30 DIV, the 0-2A lineage cells were multipolar, A2B5 +, HNK-1 +, GFAP-, and GalC-. The 0-2 lineage cells could not be distinguished as either astrocytes or oligodendrocytes on the basis of immunocytochemical or ultrastructural characteristics. These cells had dense cytoplasm, very few intermediate filaments, and a large number of vacuoles and dense bodies. The general characteristics of the cultured astrocytes at 12 DIV and 30 DIV were similar to mature and aged astrocytes in vivo, respectively. These findings suggest that the culture environment in this study accelerated aging of type 1 astrocytes. 0-2A lineage cells, on the other hand, appeared unable to differentiate into either type 2 astrocytes or oligodendrocytes when cultured in the presence of both type 1 astrocytes and fetal calf serum.

Animals↗

Subpopulations of rat cerebellar astrocytes in primary culture: morphology, cell surface antigens and [3H]GABA transport.

Glial fibrillary acidic protein (GFAP)-positive astrocytes in preconfluent cultures derived from postnatal rat cerebellum have been previously shown to display two distinct morphologies, one stellate and the other irregularly epithelioid. The immunofluorescence studies described here showed that these cells also possess unique surface characteristics. In cultures derived from 8-day-old animals stellate cells bound the monoclonal antibody A2B5 whereas the epithelioid cells bound another monoclonal antibody against rat neural antigen-2 (RAN2). Some stellate cells derived from 2-day-old animals also bound tetanus toxin. The A2B5 labelling of the stellate cells made it possible to follow their fate in vitro. In confirmation of previous time-lapse studies, they underwent a shape transformation as confluence was approached, ultimately attaining a form resembling that of the epithelioid cells. Autoradiographic transport studies using two tritiated gamma-aminobutyric acid (GABA) analogues cis-1,3-aminocyclohexane carboxylic acid (ACHC) and beta-alanine revealed further differences between the two types of astrocytes. Whereas [3H]ACHC was taken up solely by the stellate cells [3H]beta-alanine was transported by both cell types. In other experiments in which various inhibitors of [3H]GABA transport were used ACHC virtually eliminated uptake into the stellate astrocyte, but had little effect on the epithelioid ones. The 'neuron-like' [3H]GABA transport process in the stellate astrocytes was confirmed in experiments comparing the effect of another compound which has been proposed as an astrocyte-selective GABA transport inhibitor, 4,5,6,7-tetrahydroisoxazolo-(4,5-C)pyridin-3-ol (THPO). No discrimination was found in its effect on the uptake of [3H]GABA into either neurons or stellate astrocytes. Further autoradiographic studies following the uptake of [3H]GABA by postnatal cerebellar slices showed that astrocytes in all layers of the cerebellar cortex and white matter transported [3H]GABA in contrast to the situation in culture where the amino acid is taken up predominantly by the stellate astrocytes. The possibility is discussed that the stellate astrocytes represent a population of cerebellar fibrous astrocytes whereas the identity of the epithelioid astrocytes is less certain.

Amino Acids↗

Evidence for different mechanisms of induction of HSP70i: a comparison of cultured rat cortical neurons with astrocytes.

This study is a follow-up of previous work which demonstrated that cultured cortical neurons did not synthesize HSP70i immediately after heat stress when compared with cultured cortical astrocytes. We have extended the period of observation for HSP70i induction of cultured cortical neurons and astrocytes up to 24 h after heat stress. Cultured rat cortical neurons derived from 16-day-old fetal rats respond differently to heat stress than cultured rat astrocytes derived from newborn rats. They showed a delayed HSP70i induction in the majority of cultured neurons and the response was heterogeneous and was absent in most smaller neurons. The delayed neuronal induction was accompanied by a prolonged activation of heat-shock transcription factor 1 (HSF-1) and prolonged transcription of HSP70i mRNA. In comparison astrocytes showed a marked early induction of HSP70i mRNA and protein. In addition the induction of HSP70i in astrocytes was followed by translocation of the protein into the nucleus, a finding which we failed to demonstrate in neurons. Immunostaining for HSP70i was more uniform in astrocytes than neurons. Many neurons did not stain for up to 24 h after heat shock in this study. Immunocytochemical staining of HSF-1 and 2 showed major differences between neurons and astrocytes. Astrocytes showed localization of HSF-1 to the nucleus before and after heat stress, while neurons showed HSF-1 localization to the cytoplasm and nucleus before and after heat stress. Finally HSF-2 was undetectable in neurons when compared with astrocytes by Western immunoblot analysis. However, astrocytes and neurons revealed weak immunostaining of HSF-2 in the cytoplasm and nucleus. The staining in the neurons was likely secondary to cross-reactivity to an unidentified protein. We conclude that HSP70i expression after heat shock is delayed in rat cortical neurons when compared with rat cortical astrocytes. In addition most small neurons did not synthesize HSP70i after heat shock. This difference in induction of HSP70i may be secondary to localization and activation of HSF-1 but not HSF-2. Neuronal susceptibility to injury may be related to the delayed induction of HSP70i and also the possible failure of newly synthesized HSP70i to translocate into the nucleus.

Animals↗

Molecular profile of reactive astrocytes--implications for their role in neurologic disease.

The central nervous system responds to diverse neurologic injuries with a vigorous activation of astrocytes. While this phenomenon is found in many different species, its function is obscure. Understanding the molecular profile characteristic of reactive astrocytes should help define their function. The purpose of this review is to provide a summary of molecules whose levels of expression differentiate activated from resting astrocytes and to use the molecular profile of reactive astrocytes as the basis for speculations on the functions of these cells. At present, reactive astrocytosis is defined primarily as an increase in the number and size of cells expressing glial fibrillary acidic protein. In vivo, this increase in glial fibrillary acidic protein-positive cells reflects predominantly phenotypic changes of resident astroglia rather than migration or proliferation of such cells. Upon activation, astrocytes upmodulate the expression of a large number of molecules. From this molecular profile it becomes apparent that reactive astrocytes may benefit the injured nervous system by participating in diverse biological processes. For example, upregulation of proteases and protease inhibitors could help remodel the extracellular matrix, regulate the concentration of different proteins in the neuropil and clear up debris from degenerating cells. Cytokines are key mediators of immunity and inflammation and could play a critical role in the regulation of the blood-central nervous system interface. Neurotrophic factors, transporter molecules and enzymes involved in the metabolism of excitotoxic amino acids or in the antioxidant pathway may help protect neurons and other brain cells by controlling neurotoxin levels and contributing to homeostasis within the central nervous system. Therefore, an impairment of astroglial performance has the potential to exacerbate neuronal dysfunction. Based on the synopsis of studies presented, a number of issues become apparent that deserve a more extensive analysis. Among them are the relative contribution of microglia and astrocytes to early wound repair, the characterization of astroglial subpopulations, the specificity of the astroglial response in different diseases as well as the analysis of reactive astrocytes with techniques that can resolve fast physiologic processes. Differences between reactive astrocytes in vivo and primary astrocytes in culture are discussed and underline the need for the development and exploitation of models that will allow the analysis of reactive astrocytes in the intact organism.

Antibody Formation↗

Immunohistochemical staining for glial fibrillary acidic protein (GFAP) after deafferentation or ischemic infarction in rat visual system: features of reactive and damaged astrocytes.

Immunohistochemical staining for glial fibrillary acidic protein (GFAP) is standard for visualization of reactive astrocytes in tissue sections, whereas various forms of astrocytic damage remain to be described in detail. In this study we tested differences in GFAP labeling in reactive astrocytes and in glial cells damaged by ischemia and edema. Studies were performed in the anatomically well defined visual system of rat. Basic staining patterns for GFAP were established in subcortical visual nuclei and visual cortex. In the first model, deafferentation of visual centers was performed by unilateral optic nerve lesion, and characteristic changes of GFAP labeling in reactive astrocytes were studied at 0.5, 1, 1.5, 2, 4, 8 and 21 days after lesion. Initial changes were seen in the deafferented superior colliculus at 1 day after deafferentation with a diffuse increase and stellate types of reactive cells formed at 2-8 days. In the second model, small ischemic infarcts were produced in the visual cortex of rats using the method of photochemically-induced thrombosis. GFAP labeling with a polyclonal antiserum was massively enhanced in the infarct at 4 hr. Characteristic morphological changes in damaged astrocytes were seen which were also identified in experiments with simulated global ischemia. In the surround of the infarct, swelling of astrocytes also caused increased labeling. At 3-4 days infarction typical reactive astrocytes surrounded the lesioned area. In conclusion, these immunohistochemical studies on GFAP in rat visual system allow for the following classifications. (a) Normal astrocytes vary in labeling at different anatomical localizations. (b) Reactive astrocytes show enhanced labeling and larger cell-size within an interval of 1-2 days after lesion. (c) Astrocytes damaged by ischemia reveal increased labeling of disintegrating cellular elements within hours after a lesion. (d) Swollen astrocytes undergo enhanced labeling in areas with vasogenic edema.

Animals↗

Efficient presentation of myelin oligodendrocyte glycoprotein peptides but not protein by astrocytes from HLA-DR2 and HLA-DR4 transgenic mice.

The role of astrocytes in the pathogenesis of multiple sclerosis (MS) is not well understood. Astrocytes may modulate the activity of pathogenic T cells by presenting myelin antigens in combination with pro- or anti-inflammatory signals. Astrocytes have been shown to present myelin basic protein (MBP) and proteolipid protein (PLP) to T cells, but it has remained unresolved whether astrocytes present myelin oligodendrocyte glycoprotein (MOG), which has been implicated as an important autoantigen in MS. Here, we asked whether astrocytes presented MOG to T cells. To closer model presentation of human MOG by astrocytes in MS patients, we generated astrocytes from transgenic mice expressing the MS-associated MHC class II alleles HLA-DR2 (DRB1*1501) and HLA-DR4 (DRB1*0401). The results show that IFN-gamma-activated HLA-DR2 and HLA-DR4 expressing astrocytes efficiently presented immunodominant and subdominant MOG peptides to T cells. The hierarchy of the presented MOG epitopes was comparable to that of professional APCs, including dendritic cells and microglia. Importantly, astrocytes were poor at processing and presenting native MOG protein. Furthermore, astrocytes induced a mixed Th1/Th2 cytokine response in MOG-specific T cells, whereas dendritic cells induced a predominantly Th1 cell response. Collectively, the results suggest that astrocytes may modulate anti-MOG T cell responses in the CNS.

Animals↗

Astrocyte activation in working brain: energy supplied by minor substrates.

Glucose delivered to brain by the cerebral circulation is the major and obligatory fuel for all brain cells, and assays of functional activity in working brain routinely focus on glucose utilization. However, these assays do not take into account the contributions of minor substrates or endogenous fuel consumed by astrocytes during brain activation, and emerging evidence suggests that glycogen, acetate, and, perhaps, glutamate, are metabolized by working astrocytes in vivo to provide physiologically significant amounts of energy in addition to that derived from glucose. Rates of glycogenolysis during sensory stimulation of normal, conscious rats are high enough to support the notion that glycogen can contribute substantially to astrocytic glucose utilization during activation. Oxidative metabolism of glucose provides most of the ATP for cultured astrocytes, and a substantial contribution of respiration to astrocyte energetics is supported by recent in vivo studies. Astrocytes preferentially oxidize acetate taken up into brain from blood, and calculated local rates of acetate utilization in vivo are within the range of calculated rates of glucose oxidation in astrocytes. Glutamate may also serve as an energy source for activated astrocytes in vivo because astrocytes in tissue culture and in adult brain tissue readily oxidize glutamate. Taken together, contributions of minor metabolites derived from endogenous and exogenous sources add substantially to the energy obtained by astrocytes from blood-borne glucose. Because energy-generating reactions from minor substrates are not taken into account by routine assays of functional metabolism, they reflect a "hidden cost" of astrocyte work in vivo.

Acetic Acid↗

Aluminum-induced degeneration of astrocytes occurs via apoptosis and results in neuronal death.

The mechanisms by which aluminum interacts with the nervous system are only partly understood. In this study, we used cultured astrocytes and neurons to investigate the effects of long exposures to aluminum (1 mM). We found that aluminum accumulated both in neurons and astrocytes. After 8-12 days exposure, aluminum caused strong changes in the morphology of astrocytes including shrinkage of cell bodies and retraction of processes. Exposures over 15-18 days reduced astrocytes viability by 50%. Aluminum-induced degeneration of astrocytes involved the DNA fragmentation characteristic of apoptosis, and staining of aluminum-treated astrocytes with the DNA-binding fluorochrome Hoeschst 33258 revealed the typical apoptotic condensation and fragmentation of chromatin. Aluminum was also found to be neurotoxic, causing first (4-6 days) abnormal clustering and aggregation, and later (8-12 days) neuronal death. Interestingly, aluminum neurotoxicity occurred in neuroglial cultures containing approximately 10% astrocytes but not in near-pure neuronal cultures containing only 1% astrocytes. Staining of co-cultured cells with Hoeschst 33258 showed apoptotic condensation and fragmentation of chromatin in aluminum-treated astrocytes but not in co-cultured neurons. Our study demonstrates that aluminum can induce the apoptotic degeneration of astrocytes, and that this toxicity is critical in determining neuronal degeneration and death. Aluminum-mediated apoptosis of cultured astrocytes may be also a valuable model system to study the mechanisms underlying apoptosis in glial cells.

Aluminum↗

Effect of ATP on astrocyte stellation is switched from suppressive to stimulatory during development.

Adenosine 5'-triphosphate (ATP) functions as a neurotransmitter or neuromodulator in the brain. To understand the role of ATP during brain development, we investigated the effects of ATP on morphology of cultured astrocytes obtained from the cerebral cortices of embryonic day 18 (E18) and postnatal day 2 (PN2) rats. In E18 astrocytes, ATP (10-1000 microM) alone did not affect astrocyte morphology, but significantly suppressed astrocyte stellation induced by the beta-adrenoceptor agonist isoproterenol or the membrane-permeable cyclic AMP analog dibutyryl cyclic AMP. The suppressive effect of ATP in embryonic astrocytes was selectively mimicked by P2U purinoceptor agonists. ATP had no effect on stellation induced by the protein kinase C (PKC) activator phorbol ester. It is probable that ATP, via P2U purinoceptors, suppresses cyclic AMP-dependent regulatory mechanism for stellation in embryonic astrocytes. On the other hand, PN2 astrocytes differentiated into stellate cells in response to ATP. The ATP-stimulated stellation in PN2 astrocytes was mimicked by adenosine, and blocked by P1 purinoceptor antagonists. It is probable that ATP is broken down into adenosine, which stimulates P1 purinoceptors, inducing stellation in postnatal astrocytes. These findings suggest that the effect of ATP on astrocyte stellation is switched from suppressive (P2U purinoceptor-mediated) to stimulatory (P1 purinoceptor-mediated) during late embryonic to neonatal stages. ATP may be a critical factor that determines timing of astrocyte differentiation during development.

Adenine Nucleotides↗

Astrocytic neurotransmitter receptors in situ and in vivo.

In the brain, astrocytes are associated intimately with neurons and surround synapses. Due to their close proximity to synaptic clefts, astrocytes are in a prime location for receiving synaptic information from released neurotransmitters. Cultured astrocytes express a wide range of neurotransmitter receptors, but do astrocytes in vivo also express neurotransmitter receptors and, if so, are the receptors activated by synaptically released neurotransmitters? In recent years, considerable efforts has gone into addressing these issues. The experimental results of this effort have been compiled and are presented in this review. Although there are many different receptors which have not been identified on astrocytes in situ, it is clear that astrocytes in situ express a number of different receptors. There is evidence of glutamatergic, GABAergic, adrenergic, purinergic, serotonergic, muscarinic, and peptidergic receptors on protoplasmic, fibrous, or specialized (Bergmann glia, pituicytes, Müller glia) astrocytes in situ and in vivo. These receptors are functionally coupled to changes in membrane potential or to intracellular signaling pathways such as activation of phospholipase C or adenylate cyclase. The expression of neurotransmitter receptors by astrocytes in situ exhibits regional and intraregional heterogeneity and changes during development and in response to injury. There is also evidence that receptors on astrocytes in situ can be activated by neurotransmitter(s) released from synaptic terminals. Given the evidence of extra-synaptic signaling and the expression of neurotransmitter receptors by astrocytes in situ, direct communication between neurons and astrocytes via neurotransmitters could be a widespread form of communication in the brain which may affect many different aspects of brain function, such as glutamate uptake and the modulation of extracellular space.

Animals↗

Differential sensitivity of rat hippocampal and cortical astrocytes to oxygen-glucose deprivation injury.

Selective vulnerability of hippocampal neurons to ischemia is felt to relate to intense glutamatergic input and glutamate receptor expression. Since astrocytes are thought to have a neuroprotective role we speculated that hippocampal astrocyte sensitivity to insult could also contribute to this regional vulnerability. The purpose of the study was to determine if there is a differential sensitivity of cultured hippocampal and cortical astrocytes to oxygen-glucose deprivation (OGD). Hippocampal and cortical astrocytes were grown to confluence at matching cell density. Cultures were exposed to OGD for 2, 4, 6, 8 and 10 h. Progressive reduction in viability occurred in hippocampal astrocytes beginning at 2 h OGD. Reduction in cortical astrocyte viability was not observed until 4 h OGD. Death of hippocampal astrocytes was significantly greater than that of cortical astrocytes at each period of OGD. Based on acid phosphatase activity data the LD(50) for OGD duration in hippocampal astrocytes was 2 h compared to 8 h in cortical astrocytes. Regional differences in sensitivity of astrocytes to OGD implies that this may contribute to regional differences in neuronal vulnerability to ischemia.

Acid Phosphatase↗

Structural and quantitative analysis of astrocytes in the mouse hippocampus.

We revealed the structural features of astrocytes by means of light microscopy, confocal laser scanning microscopy and high voltage electron microscopy, and estimated their numerical densities in the mouse hippocampus. The high voltage electron microscope examinations of Golgi-impregnated astrocytes clearly disclosed their fine leaflet-like processes in the masses occupied by individual astrocytes. The intracellular injection of two different fluorescent tracers into two neighboring astrocytes revealed that each astrocyte occupied a discrete area with a limited overlap only at its peripheral portion. In a quantitative analysis using an optical dissector, the numerical densities of astrocytes identified as S100-immunoreactive cells were only slightly different in their areal and laminar distributions. The numerical densities were higher in the stratum lacunosum-moleculare and dentate hilus, while they were slightly lower in the principal cell layers than the average (24.2 x 10(3) mm(-3)) in whole hippocampal regions. As for the dorsoventral difference, the numerical densities were significantly larger at the ventral level in the dentate gyrus, whereas such tendency was not apparent in the hippocampus proper. The projection area of the astrocytes estimated from Golgi-impregnated samples was roughly in inverse relation to the numerical densities; the areas in the stratum lacunosum-moleculare were somewhat smaller than the other layers, where the numerical densities were high. The present study indicates that astrocytes are distributed rather evenly without any prominent areal or laminar differences and that the individual astrocytes have their own domains; the periphery of the domain of a given astrocyte is interdigitated intricately with the processes of adjacent astrocytes whereas its inner core portion is not penetrated by them.

Animals↗

Connexin-43 in rat spinal cord: localization in astrocytes and identification of heterotypic astro-oligodendrocytic gap junctions.

Connexin-43 in relation to gap junctions between astrocytes and between other cell types in rat spinal cord was investigated immunohistochemically. In gray matter, connexin-43 was distributed thoughout all laminae, but was more concentrated in the substantia gelatinosa and around the central canal. Ultrastructurally, immunostaining was present in the cytoplasm of, and at gap junctions between, fine astrocytic processes, most of which ensheathed neuronal elements. In white matter, connexin-43 was localized to somata of fibrous astrocytes, their glial fibrillary acidic protein-positive processes running parallel to myelinated axons, and at gap junctions between these processes. Labelling was also evident in thick radially-directed astrocytic processes displaying pockets of staining near immunopositive gap junctions. Near the cord surface, staining was present in cell bodies of subpial astrocytes and at gap junctions between their tangential processes which formed most of the glia limitans. Radially-directed processes of subpial astrocytes formed symmetrically- and asymmetrically-labelled gap junctions with each other and extended fine branches into surrounding white matter where they made contact and often formed gap junctions with oligodendrocytic processes at the outer surface of myelinated fibres. Immunopositive astrocyte processes also made heterologous gap junctions with unstained oligodendrocyte cell bodies. Ependymal cells lining the central canal exhibited apical cytoplasmic labelling, as well as symmetrically-labelled gap junctions at their apices. Ependymal cells also formed asymmetrically-labelled gap junctions at which the junctional membranes of unlabelled cells, presumed to be tanycytes, were unstained. The results indicate the expression of connexins in addition to connexin-43 at asymmetrically-labelled gap junctions between some astrocytic processes, between astrocytes and oligodendrocytes and between some ependymal cells. The presence of gap junctions between astrocyte and oligodendrocyte processes at the outer surface of myelin suggests incorporation of the latter into the extensive gap junctionally-coupled astrocytic syncytium.

Animals↗

Evidence for the co-localization of another connexin with connexin-43 at astrocytic gap junctions in rat brain.

Gap junctions between astrocytes as well as between astrocytes and oligodendrocytes in rat brain were immunohistochemically labelled with a monoclonal and an affinity-purified polyclonal antibody generated against connexin-26. By light microscopy, the immunolabelling patterns obtained were, with a few exceptions, remarkably similar to previously described distribution patterns of the gap junctional protein connexin-43, which is expressed by astrocytes and is localized at astrocytic gap junctions. By electron microscopy, immunoreactivity with these two anti-connexin-26 antibodies was restricted to astrocytes; inter-astrocytic gap junctional membranes were symmetrically labelled, heterologous oligo-astrocytic junctional membranes were asymmetrically labelled only on the astrocyte side and oligo-oligodendrocyte junctions were unlabelled. Two additional anti-connexin-26 antibodies that were found to produce punctate labelling in leptomeninges and liver failed to do so in brain parenchyma, consistent with reports indicating the absence of authentic connexin-26 in this tissue. Antibodies that labelled astrocytic gap junctions exhibited no cross-reaction with connexin-43 or connexin-32, as demonstrated by western blotting, but recognized liver connexin-26 as well as several brain proteins, including an approximately 32000 mol. wt protein that did not correspond to connexin-32 and a 26000 mol. wt protein that co-migrated with liver connexin-26. These results suggest that connexin-26, or more likely a protein having sequence homology with connexin-26, is targeted to astrocytic gap junctions and raise the possibility of the existence of connexins that may be co-expressed with connexin-43 in most, but perhaps not all, astrocytes.

Animals↗

Developmental regulation of glutamate transporters and glutamine synthetase activity in astrocyte cultures differentiated in vitro.

Glutamate plays an important role in brain development, physiological function, and neurodegeneration. Astrocytes control synaptic concentration of glutamate via the high affinity glutamate transporters, GLT-1 and GLAST, and the glutamate catabolizing enzyme, glutamine synthetase. In this study we show that astrocytes cultured from rat brain in various stages of development including embryonic (E18), postnatal (P1-P21) and mature (P50), show distinct patterns of GLT-1 and GLAST expression, glutamine synthetase activity, and phenotypic changes induced by dibutyryl-cyclic adenosine monophosphate. The transcripts for GLT-1 message were detectable in embryonic astrocytes only, whereas the GLAST message was highly expressed in E18 and P1-P4 astrocyte cultures, declined in P10-P21, and was undetectable in P50 astrocytes. Uptake of 3H-glutamate correlated well with GLAST expression in astrocyte cultures of all developmental stages. Glutamine synthetase activity significantly declined from high embryonic levels in P4 astrocytes and remained low throughout postnatal maturation. Exposure of astrocyte cultures to the differentiating agent, db-cAMP (250-500 microM; 6 days), resulted in a pronounced stellation, up-regulation of GLT-1 and GLAST in E18, and GLAST in P4 cultures, while it was ineffective in P10 astrocytes. By contrast, db-cAMP induced a more pronounced stimulation of glutamine synthetase activity (up to 10-fold above basal) in P10 than in E18 cultures (up to 2 times above basal). The differences in expression/inducibility of glutamate transporters and glutamine synthetase observed in astrocyte cultures derived from various stages of fetal and postnatal development suggest that astrocytes in vivo might also respond differently to environmental or injurious stimuli during development and maturation.

ATP-Binding Cassette Transporters↗

Immature astrocytes in Fukuyama congenital muscular dystrophy: an immunohistochemical study.

Recent studies of Fukuyama congenital muscular dystrophy have focused on abnormalities of the basement membrane in muscle and brain. The cerebral cortex has a unique basement membrane at the glia limitans, which is intimately related to astrocytes in the developing brain, and the basement membrane may be partially produced by the astrocyte. In this study the cerebral astrocytes in six patients with Fukuyama congenital muscular dystrophy, including two fetal patients, were characterized by immunohistochemical study. In fetal Fukuyama congenital muscular dystrophy, astrocytes reacted less to antibodies of glial fibrillary acidic protein, S-100 protein, and alphaB-crystallin than control astrocytes, but in postnatal Fukuyama congenital muscular dystrophy, astrocytes reacted more to these antibodies and displayed beading of processes. Moreover, vimentin was positive in the astrocytes of two postnatal Fukuyama congenital muscular dystrophy patients. This astrocytic appearance may suggest immaturity of astrocytes in Fukuyama congenital muscular dystrophy. Astrocytes exhibiting beaded cytoplasmic processes were prominent at the subpia of the cortex and around vessels. The authors hypothesize that these immature astrocytes are unable to participate in the function of the cortical basement membrane, which is defective in Fukuyama congenital muscular dystrophy. Studies of neurons and meninges were similar to those of control subjects.

Adolescent↗