Acarin Laia, Peluffo Hugo, Barbeito Luis, Castellano Bernardo, González Berta
Unit of Histology, School of Medicine, Department of Cell Biology, Physiology and Immunology, Institute of Neurosciences, Universitat Autonoma Barcelona, Bellaterra 08193, Spain.
J Neurotrauma. 2005 Jan;22(1):189-200. doi: 10.1089/neu.2005.22.189.
Oxygen free radicals and nitric oxide (NO) participate in the pathogenesis of acute central nervous system (CNS) injury by forming peroxynitrite, which promotes oxidative damage and tyrosine nitration. Neuronal nitration is associated with cell death, but little is known of the characteristics and cell fate of nitrated astrocytes. In this study, we have used a postnatal excitotoxic lesion model (intracortical NMDA injection) and our aims were (i) to evaluate the temporal and spatial pattern of astroglial nitration in correlation with the neuropathological process and the sources of NO; and (ii) to establish, if any, the correlation among astrocyte nitration and other events such as expression of cytoskeletal proteins, antioxidant enzymes, and cell death markers to cope with nitration and/or undergo cell death. Our results show that after postnatal excitotoxic damage two distinct waves of nitration were observed in relation to astrocytes. At 24 h post-lesion, early-nitrated astrocytes were found within the neurodegenerating area, coinciding with the time of maximal cell death. These early-nitrated astrocytes are highly ramified protoplasmic cells, showing diffuse glial fibrillary acidic protein (GFAP) content and expressing inducible NOS. At later time-points, when astrogliosis is morphologically evident, nitrated hypertrophied reactive astrocytes are observed in the penumbra and the neurodegenerated area, displaying increased expression of GFAP and vimentin cytoskeletal proteins and of metallothionein I-II and Cu/Zn superoxide dismutase antioxidant proteins. Moreover, despite revealing activated caspase-3, they do not show TUNEL labeling. In summary, we show that nitrated astrocytes in vivo constitute a subpopulation of highly reactive astrocytes which display high resistance towards oxidative stress induced cell death.
氧自由基和一氧化氮(NO)通过形成过氧亚硝酸盐参与急性中枢神经系统(CNS)损伤的发病机制,过氧亚硝酸盐会促进氧化损伤和酪氨酸硝化。神经元硝化与细胞死亡有关,但对于硝化星形胶质细胞的特征和细胞命运知之甚少。在本研究中,我们使用了出生后兴奋性毒性损伤模型(皮质内注射NMDA),我们的目的是:(i)评估星形胶质细胞硝化的时空模式与神经病理过程和NO来源的相关性;(ii)确定星形胶质细胞硝化与其他事件(如细胞骨架蛋白、抗氧化酶和细胞死亡标志物的表达)之间是否存在相关性,以应对硝化和/或经历细胞死亡。我们的结果表明,出生后兴奋性毒性损伤后,观察到与星形胶质细胞相关的两个不同的硝化波。损伤后24小时,在神经退行性变区域发现早期硝化的星形胶质细胞,与最大细胞死亡时间一致。这些早期硝化的星形胶质细胞是高度分支的原浆细胞,显示出弥漫性胶质纤维酸性蛋白(GFAP)含量,并表达诱导型一氧化氮合酶。在后期,当星形胶质细胞增生在形态上明显时,在半暗带和神经退行性变区域观察到硝化的肥大反应性星形胶质细胞,显示GFAP和波形蛋白细胞骨架蛋白以及金属硫蛋白I-II和铜/锌超氧化物歧化酶抗氧化蛋白的表达增加。此外,尽管显示活化的半胱天冬酶-3,但它们未显示TUNEL标记。总之,我们表明体内硝化的星形胶质细胞构成了高度反应性星形胶质细胞的一个亚群,它们对氧化应激诱导的细胞死亡具有高度抗性。