Intermediate AGN feedback models in FLAMINGO simulations best match X-GAP observations of hot gas in galaxy groups, with fgas-2sigma showing 0.8sigma tension and fgas-8sigma ruled out at over 4sigma.
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Bound or blown: the fate of hot gas in galaxy groups
Intermediate AGN feedback models in FLAMINGO simulations best match X-GAP observations of hot gas in galaxy groups, with fgas-2sigma showing 0.8sigma tension and fgas-8sigma ruled out at over 4sigma.