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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
* BH mass at fixed bulge mass at high z is higher than low z, as recently found in some z>6 quasars by Feige Wang & Xiaohui Fan, using ALMA data. * SF in supergiant shells at high z has been overlooked. Where will these stars go? moving together to the central region, or distributed more widely?
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
