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应激蛋白与原位及半胱胺处理的神经胶质细胞培养物中自发荧光星形胶质细胞内含物的共定位。

Stress protein co-localization to autofluorescent astrocytic inclusions in situ and in cysteamine-treated glial cultures.

作者信息

Mydlarski M B, Schipper H M

机构信息

Bloomfield Centre for Research in Aging, Lady Davis Institute for Medical Research, Sir Mortimer B. Davis-Jewish General Hospital, Que., Canada.

出版信息

Brain Res. 1993 Nov 5;627(1):113-21. doi: 10.1016/0006-8993(93)90754-b.

Abstract

In the aging brain, a unique subpopulation of limbic and periventricular astrocytes accumulates red autofluorescent, peroxidase-positive cytoplasmic inclusions distinct from lipofuscin. Cysteamine (CSH) exposure rapidly induces identical inclusions in cultured, immature astroglia. CSH induces a cellular stress response prior to astrocyte granulation. To determine whether stress proteins are actual constituents of the autofluorescent granules, 12-week-old rat brain sections and CSH-treated astroglial cultures were immunostained with various anti-stress protein antibodies and evaluated by laser scanning confocal microscopy. We observed intense co-localization of heat shock protein (HSP) 27 and ubiquitin (Ub) to the autofluorescent astrocyte granules in situ and in CSH-treated glial cultures. In both preparations, glucose regulated protein (GRP) 94 consistently exhibited partial co-localization to the granule periphery and adjacent cytoplasm. In contrast, HSP72 co-localization to these inclusions was only occasionally seen and the granules appeared entirely devoid of HSP90 and alpha B-crystallin. Acute exposure of cultured astroglia to CSH induced intense cytoplasmic Ub staining, suggesting that activation of the Ub pathway may be an early event in the biogenesis of these astrocytic granules. Taken together, our results support the notion that the autofluorescent astrocyte inclusions are stress or heat shock granules which progressively accumulate in the aging periventricular brain. Moreover, CSH greatly accelerates the appearance of this senescent astrocyte phenotype in primary culture.

摘要

在衰老的大脑中,边缘和脑室周围星形胶质细胞的一个独特亚群会积累红色自发荧光、过氧化物酶阳性的细胞质内含物,这些内含物不同于脂褐素。用半胱胺(CSH)处理培养的未成熟星形胶质细胞,可迅速诱导出相同的内含物。CSH在星形胶质细胞形成颗粒之前会诱导细胞应激反应。为了确定应激蛋白是否是自发荧光颗粒的实际成分,我们用各种抗应激蛋白抗体对12周龄大鼠脑切片和经CSH处理的星形胶质细胞培养物进行免疫染色,并通过激光扫描共聚焦显微镜进行评估。我们观察到热休克蛋白(HSP)27和泛素(Ub)在原位以及经CSH处理的胶质细胞培养物中与星形胶质细胞的自发荧光颗粒强烈共定位。在这两种制剂中,葡萄糖调节蛋白(GRP)94始终在颗粒周边和相邻细胞质中呈现部分共定位。相比之下,HSP72与这些内含物的共定位仅偶尔可见,且颗粒似乎完全没有HSP90和αB晶状体蛋白。培养的星形胶质细胞急性暴露于CSH会诱导强烈的细胞质Ub染色,这表明Ub途径的激活可能是这些星形胶质细胞颗粒生物发生的早期事件。综上所述,我们的结果支持这样一种观点,即星形胶质细胞的自发荧光内含物是应激或热休克颗粒,它们在衰老的脑室周围大脑中逐渐积累。此外,CSH在原代培养中极大地加速了这种衰老星形胶质细胞表型的出现。

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