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wiki:scratch [2021/01/07 02:32] Cheng Li created |
wiki:scratch [2021/01/08 01:57] (current) Cheng Li |
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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 | + | ====== Headline ====== |
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+ | ===== Li Hui ===== | ||
+ | |||
+ | * Does the IMF differ between the two modes of star formation? | ||
+ | * steeper mass function of star clusters by major mergers; is this consistent with the linear relation of halo mass and GC total mass? | ||
+ | * triple distribution in the Age-Metallicity diagram? due to major mergers? | ||
+ | |||
+ | ===== Ma Xiangcheng ===== | ||
+ | |||
+ | |||
+ | * low-mass galaxies: what about their SFH? | ||
+ | * 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 | ||
+ | |||
+ | * What's the role of mergers, and bars? | ||
+ | * 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? | ||
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GCs form efficiently in gas-rich, turbulent ISM, Ma+20a, MNRAS, 493, 4315 | GCs form efficiently in gas-rich, turbulent ISM, Ma+20a, MNRAS, 493, 4315 | ||
- | SF in supergiant shells at high z has been overlooked. | + | |