星形胶质细胞在肝性脑病中的作用。

M D Norenberg
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引用次数: 218

摘要

阿尔茨海默病II型星形胶质细胞改变是人类和实验动物在肝性脑病(HE)发生时大脑中独特的形态学改变。这种改变是HE发病机制中的主要事件,还是继发于中枢神经系统其他部分的损伤,目前尚不清楚。在大鼠HE模型中的研究显示,星形胶质细胞的早期反应性变化以细胞质肥大为特征。在后期阶段,退行性变化随之而来,与光学显微镜观察到的阿尔茨海默氏II型变化相对应。鉴于星形胶质细胞在氨解毒中的作用以及氨在HE发病机制中的重要性,我们认为星形胶质细胞的初始变化是氨解毒的形态学相关因素。我们推测,后期的退行性改变可能导致星形胶质细胞无法完成关键功能(如神经递质摄取、离子调节等),从而导致脑病的发生。最近,星形胶质细胞在HE中的潜在参与被进一步研究,使用原代星形胶质细胞培养。将培养物暴露于临床相关浓度的氨中,其形态变化与在体内实验HE中观察到的非常相似。这些有害的影响可以通过提高细胞中循环AMP的水平来部分预防。其他潜在的毒素(辛酸、苯酚)也表现出病理变化。虽然这三个人都有一些共同的改变,但他们每个人都有不同的病理影响。还证实了与这些毒素的协同相互作用。氨处理的星形胶质细胞的功能研究表明:低剂量或短期暴露时,K+、谷氨酸和GABA的吸收保持不变或略有增加,而高剂量或长时间暴露时,这些活动减少。随着氨处理时间的延长,ATP值出现下降。初步研究结果显示,除了受体亲和力略有下降外,β -肾上腺素能受体没有明显紊乱。然而,异丙肾上腺素刺激后,环AMP的产生减少。发现苯二氮受体的数量略有增加。这些研究表明,暴露于氨和其他假定的毒素后,星形胶质细胞发生了深刻的变化。有人提出,参与HE沉淀的毒素和因素是通过影响星形胶质细胞的特性来实现的。这些特性的紊乱可能导致神经胶质功能障碍(原发性神经胶质病),导致脑病状态。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The role of astrocytes in hepatic encephalopathy.

The Alzheimer type II astrocyte change is the distinctive morphologic alteration in brain of humans and experimental animals succumbing to hepatic encephalopathy (HE). Whether this change is a primary event in the pathogenesis of HE or whether it is secondary to injury of some other component(s) of the CNS has not been clarified. Studies in a rat model of HE have revealed early reactive changes in astrocytes characterized by cytoplasmic hypertrophy. During the later phases, degenerative changes ensue corresponding to the Alzheimer type II change observed by light microscopy. In view of the role of astrocytes in ammonia detoxification and the importance of ammonia in the pathogenesis of HE, we have suggested that the initial astrocytic changes are the morphological correlates of ammonia detoxification. We have speculated that the later degenerative alterations could lead to failure by astrocytes to carry out key functions (e.g., neurotransmitter uptake, ion regulation, and the like) and contribute the development of the encephalopathy. Recently, the potential involvement of astrocytes in HE has been further investigated, using primary astrocyte cultures. Exposure of cultures to ammonia at clinically relevant concentrations has shown morphologic changes closely resembling those observed in experimental HE in vivo. These deleterious effects can partly be prevented by raising cyclic AMP levels in cells. Other potential toxins (octanoic acid, phenol) have shown pathologic changes as well. Although some alterations were common to all three, they each possessed distinctive pathological effects. A synergistic interaction has also been demonstrated with these toxins. Functional studies of ammonia-treated astrocytes have shown the following: With low doses or short-term exposure, the uptakes of K+, glutamate, and GABA remained unchanged or slightly increased, whereas with higher doses or longer treatment, those activities diminished. A fall in ATP values occurred with prolonged ammonia treatment. Preliminary findings have shown no significant derangements in the beta-adrenergic receptor, except for a slight decrease in receptor affinity. However, cyclic AMP production was diminished following stimulation with isoproterenol. A slight rise in the number of benzodiazepine receptors was found. These studies indicate that profound changes occur in astrocytes following exposure to ammonia and other putative toxins. It is proposed that toxins and factors involved in the precipitation of HE do so by affecting astroglial properties. Derangements in such properties may lead to glial dysfunction (primary gliopathy), resulting in an encephalopathic state.

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