Neuroscience Research Center, Kerman, Iran.
Brain Res Bull. 2010 Jan 15;81(1):43-52. doi: 10.1016/j.brainresbull.2009.11.002.
Although there are some similarities in the molecular and cellular pattern of Wallerian degeneration in the PNS and CNS, in the CNS the removal of axonal and myelin debris by microglia and astrocytes is not very efficient and occurs over a much longer time frame than seen in a peripheral nerve. Several animal models have been used to study Wallerian degeneration-induced glial reactivity in the CNS and PNS. Although these models have clarified some aspects of the mechanisms underlying the differential glial cell responses in the PNS and CNS, they do not lend themselves easily to deciphering the mechanisms governing the location and extent of Wallerian degeneration-induced CNS glial reactivity. The present study develops a new animal model that entails destruction of the left sensorimotor cortex of adult rats to induce Wallerian degeneration within the total length of a fiber tract (i.e. the dorsal corticospinal tract) that extends all the way from the cerebral cortex to the sacral level of the spinal cord. Since the axonal degeneration in the ventral medulla and dorsal funiculus of the spinal cord would be confined to the corticospinal tract, it was predicted the glial reactivity would also be restricted to this fiber tract. Three distinct proximal-distal levels of this pathway were examined to determine the morphology, distribution and immunophenotype of microglia and astrocytes between 1 day and 16 weeks after sensorimotor cortex aspiration. As expected, there was a proximal to distal gradient in the appearance of glial reactivity along the length of the pathway, with the microglial reactivity being seen as early as 3 weeks in the left pyramid, and by 4 weeks (i.e. at C6) and 6 weeks (i.e. at T11) in the right dorsal corticospinal tract. Astrocytic reactivity lagged behind that of the microglial response at each level of the pathway. The microglial and astrocytic reactivity persisted up to 16 weeks after cortical injury, which was the longest survival time studied. The sensorimotor cortex aspiration model should prove extremely useful in deciphering the molecular mechanisms controlling Wallerian degeneration-induced CNS glial reactivity and in determining the relative role of astrocytes vs microglia in clearance of axonal and myelin debris.
虽然周围神经系统和中枢神经系统的 Wallerian 变性在分子和细胞模式上存在一些相似之处,但在中枢神经系统中,小胶质细胞和星形胶质细胞清除轴突和髓鞘碎片的效率并不高,而且发生的时间比周围神经长得多。已经使用了几种动物模型来研究中枢神经系统和周围神经系统中 Wallerian 变性诱导的神经胶质反应。尽管这些模型阐明了周围神经系统和中枢神经系统中神经胶质细胞反应差异的一些机制,但它们不容易用于破译控制 Wallerian 变性诱导的中枢神经系统神经胶质反应的位置和程度的机制。本研究开发了一种新的动物模型,该模型涉及破坏成年大鼠的左侧感觉运动皮层,以诱导全长纤维束(即背侧皮质脊髓束)中的 Wallerian 变性,该纤维束从大脑皮层延伸至脊髓的骶骨水平。由于脊髓腹侧髓质和背侧束中的轴突变性仅限于皮质脊髓束,因此预计神经胶质反应也将局限于该纤维束。在感觉运动皮层抽吸后 1 天至 16 周内,检查了该途径的三个不同的近-远水平,以确定小胶质细胞和星形胶质细胞的形态、分布和免疫表型。正如预期的那样,沿着途径的长度存在从近端到远端的神经胶质反应梯度,左侧锥体中的小胶质细胞反应早在 3 周时就出现,而在 4 周(即 C6)和 6 周(即 T11)时在右侧背侧皮质脊髓束中出现。星形胶质细胞反应在途径的每个水平都落后于小胶质细胞反应。小胶质细胞和星形胶质细胞反应持续到皮质损伤后 16 周,这是研究的最长存活时间。感觉运动皮层抽吸模型应该非常有助于破译控制 Wallerian 变性诱导的中枢神经系统神经胶质反应的分子机制,并确定星形胶质细胞与小胶质细胞在清除轴突和髓鞘碎片方面的相对作用。