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人类胎儿大脑中的放射状胶质细胞:一项高尔基染色、免疫荧光和电子显微镜联合研究

Radial glia in the human fetal cerebrum: a combined Golgi, immunofluorescent and electron microscopic study.

作者信息

Choi B H, Lapham L W

出版信息

Brain Res. 1978 Jun 16;148(2):295-311. doi: 10.1016/0006-8993(78)90721-7.

Abstract

Golgi techniques, immunofluorescence for glial fibrillary acidic (GFA) protein, and electron microscopy (EM) were used to determine the nature of radial glia in the cerebrum of human fetuses ranging from 7 to 20 weeks of ovulation age. Successful Golgi impregnation of radial fibers was achieved in fetuses 12 weeks of age and older. These fibers spanned the entire thickness of the hemisphere. At the pial surface many of them branched and terminated in pyramidal end feet expansions. Indirect immunofluorescent preparations utilizing antiserum to GFA protein, a protein specific for astrocytes, demonstrated numerous radially oriented nearly parallel fluorescent fibres between the ventricular zone and pia mater. GFA protein-positive fibers were demonstrated in all fetal specimens examined with this technique (10 weeks of age and older). Along the outer border of the marginal zone they formed a horizontal GFA protein-containing subpial membrane. By EM there were numerous linear electron lucent astrocytic processes containing 8-9 nm filaments and occasional glycogen granules at all levels of the cerebrum. They were interspersed among smaller and darker neuronal processes containing 20-25 nm neurotubules, and were demonstrable at all fetal ages between 7 and 18 weeks. They formed pericapillary investments and subpial terminal expansions closely abutting basal lamina of pia mater in every specimen examined. On the basis of these combined analyses, we conclude that radial glial fibers in early human fetal cerebrum represent processes of immature astrocytes. Although subsequently undergoing further maturation, radial glia already possess fundamental immunocytochemical and morphological characteristics indicative of astrocytic differentiation. A significant implication of our findings is that the development of astrocytes in the human fetal brain occurs much earlier than formerly believed.

摘要

运用高尔基染色技术、胶质纤维酸性蛋白(GFA)免疫荧光法以及电子显微镜(EM),来确定排卵年龄在7至20周的人类胎儿大脑中放射状胶质细胞的性质。12周及以上胎儿的放射状纤维成功实现了高尔基染色。这些纤维贯穿半球的整个厚度。在软脑膜表面,它们中的许多分支并终止于锥体状终足扩张处。利用抗星形胶质细胞特异性蛋白GFA的抗血清进行间接免疫荧光制片,结果显示在脑室区和软脑膜之间有许多呈放射状排列且近乎平行的荧光纤维。用该技术检测的所有胎儿标本(10周及以上)中均显示出GFA蛋白阳性纤维。沿着边缘区的外边界,它们形成了一层含GFA蛋白的水平软脑膜下膜。通过电子显微镜观察,在大脑各层面均有大量含8 - 9纳米细丝和偶尔糖原颗粒的线性电子透明星形胶质细胞突起。它们散布于含有20 - 25纳米神经微管的较小且较暗的神经元突起之间,在7至18周的所有胎儿期均可显示。在每个检测标本中,它们形成了紧密邻接软脑膜基膜的毛细血管周围包绕结构和软脑膜下终末扩张。基于这些综合分析,我们得出结论,人类胎儿早期大脑中的放射状胶质纤维代表未成熟星形胶质细胞的突起。尽管放射状胶质细胞随后会进一步成熟,但它们已经具备了指示星形胶质细胞分化的基本免疫细胞化学和形态学特征。我们研究结果的一个重要意义在于,人类胎儿大脑中星形胶质细胞的发育比之前认为的要早得多。

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