The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
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DOI: 10.1093/mnras/stz1494
Abstract: The quenching ‘maintenance’ and related ‘cooling flow’ problems are important in galaxies from Milky Way mass through clusters. We investigate this in haloes with masses ∼$10^{12}\!-\!10^{14}\, {\rm M}_{\odot }$, using non-cosmological high-resolution hydrodynamic simulations with… read more here.
Keywords: magnetic fields; morphological quenching; feedback; stellar feedback ... See more keywords