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low-mass galaxies: what about their SFH? What's the role of mergers, and bars?

turbulent SF suppress SMBH growth? What if in case of mergers? the result seems to be quite different from those predicted by Volker's simulations

diverse kinematics + metallicity gradients at z~2. Xiacheng Ma+2017b, MNRAS, 466, 4780

HiZFIRE, Ma+18a

GCs form efficiently in gas-rich, turbulent ISM, Ma+20a, MNRAS, 493, 4315

SF in supergiant shells at high z has been overlooked.

wiki/scratch.1609986761.txt.gz · Last modified: 2021/01/07 02:32 by Cheng Li