This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
wiki:scratch [2021/01/07 02:36] Cheng Li |
wiki:scratch [2021/01/08 01:57] (current) Cheng Li |
||
---|---|---|---|
Line 1: | Line 1: | ||
- | 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 ====== |
+ | ===== 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. | * 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? | * 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? |