论文标题

黑洞 - 盖拉克斯共同进化和反馈的作用

Black hole-galaxy co-evolution and the role of feedback

论文作者

Capelo, Pedro R., Feruglio, Chiara, Hickox, Ryan C., Tombesi, Francesco

论文摘要

活跃的银河核(AGN)通过复杂的喂食和反馈相互作用来积聚与宿主星系共同发展的超大质量黑洞。在本章中,我们首先讨论了相互作用和孤立系统中星系中的AGN加油,重点介绍了不稳定性在气体预算的角度动量预算中的作用。然后,我们通过AGN驱动的风从核-PC缩放到银河系和圆形培养基尺度的观察结果和反馈模型。我们继续概述AGN人群的调查和统计特性,然后最后讨论了未来设施的前景,特别是雅典娜。

Active galactic nuclei (AGN) are accreting supermassive black holes co-evolving with their host galaxies through a complex interplay of feeding and feedback. In this chapter, we first discuss AGN fuelling in galaxies, both in interacting and isolated systems, focusing on the role that instabilities have on the angular momentum budget of the gas. We then review observations and models of feedback through AGN-driven winds from nuclear, sub-pc scales out to galactic and circumgalactic medium scales. We continue with an overview of surveys and statistical properties of the AGN population, before concluding with a discussion on the prospects for the future facilities, focusing in particular on Athena.

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