Observed passive fractions of local central galaxies track stellar and bulge mass, but the L-GALAXIES and SAGE simulations predict passive fractions driven by halo, black hole, and bulge properties, leaving clear tensions with SDSS data.
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On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
Observed passive fractions of local central galaxies track stellar and bulge mass, but the L-GALAXIES and SAGE simulations predict passive fractions driven by halo, black hole, and bulge properties, leaving clear tensions with SDSS data.