Neurobiology Section, Division of Biological Sciences, University of California, San Diego, La Jolla, California, USA.
J Neurochem. 2013 Dec;127(5):632-43. doi: 10.1111/jnc.12436. Epub 2013 Sep 30.
Astrocytes, an abundant form of glia, are known to promote and modulate synaptic signaling between neurons. They also express α7-containing nicotinic acetylcholine receptors (α7-nAChRs), but the functional relevance of these receptors is unknown. We show here that stimulation of α7-nAChRs on astrocytes releases components that induce hippocampal neurons to acquire more α-amino-3-hydroxy-5-methyl-4-isoxazolepropionic acid (AMPA) receptors post-synaptically at glutamatergic synapses. The increase is specific in that no change is seen in synaptic NMDA receptor clusters or other markers for glutamatergic synapses, or in markers for GABAergic synapses. Moreover, the increases in AMPA receptors on the neuron surface are accompanied by increases in the frequency of spontaneous miniature synaptic currents mediated by the receptors and increases in the ratio of evoked synaptic currents mediated by AMPA versus NMDA receptors. This suggests that stimulating α7-nAChRs on astrocytes can convert 'silent' glutamatergic synapses to functional status. Astrocyte-derived thrombospondin is necessary but not sufficient for the effect, while tumor necrosis factor-α is sufficient but not necessary. The results identify astrocyte α7-nAChRs as a novel pathway through which nicotinic cholinergic signaling can promote the development of glutamatergic networks, recruiting AMPA receptors to post-synaptic sites and rendering the synapses more functional. We find that activation of nicotinic receptors on astrocytes releases a component that specifically recruits AMPA receptors to glutamatergic synapses. The recruitment appears to occur preferentially at what may be 'silent synapses', that is, synapses that have all the components required for glutamatergic transmission (including NMDA receptors) but lack sufficient AMPA receptors to generate a response. The results are unexpected and open up new possibilities for mechanisms underlying network formation and synaptic plasticity.
星形胶质细胞是一种丰富的神经胶质细胞,已知其可以促进和调节神经元之间的突触信号传递。它们还表达含有α7 亚基的烟碱型乙酰胆碱受体(α7-nAChRs),但这些受体的功能相关性尚不清楚。我们在这里表明,星形胶质细胞上的α7-nAChR 被刺激后会释放出一些成分,这些成分诱导海马神经元在后突触水平在谷氨酸能突触上获得更多的α-氨基-3-羟基-5-甲基-4-异恶唑丙酸(AMPA)受体。这种增加是特异性的,因为在突触 NMDA 受体簇或其他谷氨酸能突触标志物,或 GABA 能突触标志物上没有看到变化。此外,神经元表面上 AMPA 受体的增加伴随着受体介导的自发性微小突触电流频率的增加,以及 AMPA 受体介导的诱发突触电流与 NMDA 受体介导的诱发突触电流的比率增加。这表明刺激星形胶质细胞上的α7-nAChR 可以将“沉默”的谷氨酸能突触转化为功能状态。星形胶质细胞衍生的血栓素是必需的,但不是充分的,而肿瘤坏死因子-α是充分的,但不是必需的。结果表明,星形胶质细胞 α7-nAChR 是尼古丁胆碱能信号传递促进谷氨酸能网络发育的新途径,将 AMPA 受体募集到后突触位点,并使突触更具功能性。我们发现,星形胶质细胞上的烟碱受体的激活会释放一种特定的成分,将 AMPA 受体募集到谷氨酸能突触。这种募集似乎优先发生在可能是“沉默突触”的部位,即具有谷氨酸能传递所需的所有成分(包括 NMDA 受体)但缺乏足够的 AMPA 受体以产生反应的突触。这些结果出人意料,为网络形成和突触可塑性的潜在机制开辟了新的可能性。