Marín-Padilla M
Department of Pathology, Dartmouth Medical School, Hanover, New Hampshire 03755, USA.
J Comp Neurol. 1995 Jul 10;357(4):554-72. doi: 10.1002/cne.903570407.
The prenatal developmental histories of layer I, fibrous (white matter), and protoplasmic (gray matter) astrocytes have been studied in the human neocortex by the rapid Golgi method. The developmental route followed by each of these astrocytes is a distinct process which evolves from a specific precursor, occurs at a different time, and is linked to a specific event. The differentiation of layer I astrocytes is linked to the neocortex external glial limiting membrane (EGLM), that of fibrous astrocytes to the early white matter vascularization and maturation, and that of protoplasmic astrocytes to the late gray matter ascending vascularization and maturation. At the start of development, three glial precursors are established in the neocortex: 1) original radial neuroectodermal cells with nuclei above the primordial plexiform layer (PPL) by losing their ependymal and retaining their pial attachments become early astrocytes of layer I and EGLM components; 2) neuroectodermal cells with nuclei below the PPL that retain their pial and ependymal attachments become type I radial glial cells which are committed to the guidance of neurons and the early EGLM maintenance; and, 3) neuroectodermal cells that lose their pial but retain their ependymal attachment are transformed into type II radial glial precursors. By progressively losing their ependymal attachment, type II radial glia precursors become freely migrating cells, establish vascular contacts, and differentiate into fibrous astrocytes (and into oligodendrocytes?) throughout the subplate, developing white matter, and paraventricular regions. After the formation of the gray matter, additional layer I astrocytes are needed for the EGLM late prenatal and postnatal maintenance because type I radial glia cells start to regress and to reabsorb their EGLM endfeet. A late ependyma-to-pia migration of glial precursors progressively repopulates layer I with additional astrocytes and establishes the ephemeral subpial granular layer (SGL) of Ranke. From the 15th week of gestation to the time of birth, late astrocytes of layer I lose their EGLM attachments, migrate freely into the maturing gray matter, establish vascular contacts, and differentiate into protoplasmic astrocytes. The protoplasmic astrocytes of the gray matter evolve from transformation of layer I astrocytes rather than from radial glia cells as is generally believed.
通过快速高尔基方法,对人类新皮质中I层、纤维性(白质)和原浆性(灰质)星形胶质细胞的产前发育史进行了研究。这些星形胶质细胞各自遵循的发育途径是一个独特的过程,它从特定的前体细胞演化而来,发生在不同的时间,并与特定事件相关联。I层星形胶质细胞的分化与新皮质外胶质界膜(EGLM)相关,纤维性星形胶质细胞的分化与早期白质血管形成和成熟相关,原浆性星形胶质细胞的分化与晚期灰质上升血管形成和成熟相关。在发育开始时,新皮质中建立了三种胶质前体细胞:1)原始的放射状神经外胚层细胞,其细胞核位于原始丛状层(PPL)上方,通过失去室管膜并保留软膜附着,成为I层早期星形胶质细胞和EGLM成分;2)细胞核位于PPL下方且保留软膜和室管膜附着的神经外胚层细胞,成为I型放射状胶质细胞,其负责引导神经元和维持早期EGLM;3)失去软膜但保留室管膜附着的神经外胚层细胞转变为II型放射状胶质前体细胞。通过逐渐失去室管膜附着,II型放射状胶质前体细胞成为自由迁移的细胞,建立血管联系,并在整个板下、发育中的白质和室周区域分化为纤维性星形胶质细胞(以及少突胶质细胞?)。在灰质形成后,由于I型放射状胶质细胞开始退化并重新吸收其EGLM终足,EGLM在产前后期和产后维持需要额外的I层星形胶质细胞。胶质前体细胞从室管膜到软膜的晚期迁移逐渐使I层重新充满额外的星形胶质细胞,并建立了短暂的兰克软膜下颗粒层(SGL)。从妊娠第15周直到出生,I层晚期星形胶质细胞失去其EGLM附着,自由迁移到成熟的灰质中,建立血管联系,并分化为原浆性星形胶质细胞。灰质中的原浆性星形胶质细胞是由I层星形胶质细胞转变而来,而不是如普遍认为的那样由放射状胶质细胞分化而来。