Black hole feedback sets an entropy ceiling in halos enabling buoyant outflows with mass-independent entropy at the virial radius in simulations, predicting star formation rejuvenation above M_crit ~ 10^13.5-14 solar masses.
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Thermostats, Not Engines: A New Picture of Halo Gas Regulation
Black hole feedback sets an entropy ceiling in halos enabling buoyant outflows with mass-independent entropy at the virial radius in simulations, predicting star formation rejuvenation above M_crit ~ 10^13.5-14 solar masses.