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The limits of feedback from active galactic nuclei

astro-ph.GA · 2026-05-15 · unverdicted · novelty 6.0

AGN feedback creates a mass-independent entropy ceiling that allows outflows to escape halos only below M_200m = 10^13.7 M_sun, explaining depleted gas in groups versus near-cosmic fractions in clusters.

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  • The limits of feedback from active galactic nuclei astro-ph.GA · 2026-05-15 · unverdicted · none · ref 12

    AGN feedback creates a mass-independent entropy ceiling that allows outflows to escape halos only below M_200m = 10^13.7 M_sun, explaining depleted gas in groups versus near-cosmic fractions in clusters.