Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions

Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions

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In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modelling of feedback from active galactic nuclei (AGNs). The amount of energy released by AGN feedback is proportional to the mass that has been accreted on to the black holes (BHs), but t...

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Bibliographic Details
Main Authors: Habouzit, Mélanie (Author), Somerville, Rachel S (Author), Li, Yuan (Author), Genel, Shy (Author), Aird, James (Author), Anglés-Alcázar, Daniel (Author), Davé, Romeel (Author), Georgiev, Iskren Y (Author), McAlpine, Stuart (Author), Rosas-Guevara, Yetli (Author), Dubois, Yohan (Author), Nelson, Dylan (Author), Banados, Eduardo (Author), Hernquist, Lars (Author), Peirani, Sébastien (Author), Vogelsberger, Mark (Author)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-05-06T17:44:38Z.
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