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Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback

By Samuel Ruthven Ward and others
Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the quenching of massive galaxies in the vast majority of modern galaxy evolution models. However, direct observational evidence that AGN feedback causes quenching on a population scale is lacking. Studies have shown that luminous AGN are preferentially located... Show more
April 28, 2022
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Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
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