Difference between revisions of "星系尺度的演化"
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*members：常瑞香，富坚，沈世银，赵东海 | *members：常瑞香，富坚，沈世银，赵东海 | ||
==讨论== | ==讨论== | ||
===2022/09/22=== | |||
*赵：[[:File:2206.11913.pdf |angular_momentum controlled by cosmological initial condition]] | |||
*富：[[:File:2209.01720.pdf |xGASS:connection between j and M]] | |||
*钟：会议记录 [[:File:星系尺度小组讨论0922.doc|record0922]] | |||
===2022/09/01=== | ===2022/09/01=== | ||
Latest revision as of 02:04, 22 September 2022
- members：常瑞香，富坚，沈世银，赵东海
讨论
2022/09/22
- 赵：angular_momentum controlled by cosmological initial condition
- 富：xGASS:connection between j and M
- 钟：会议记录 record0922
2022/09/01
- 富：HI_and_angular_momentum
- 富：IAU 2018 FM6角动量分会会议文集
- 常：厚盘 Bournaud 2009 ApJ 694 L158
- 常：厚盘 Bournaud 2009 ApJ 707 L1
- 钟：会议记录 record0901
2022/08/18
2022/07/11
- 赵：spin transfer
- 沈：unified model from Krumholz18
- 钟：会议记录 record0711
2022/06/27
- 富： ppt
- 钟：会议记录 record0627
to do
- 沈：收集MaNGA中气体盘和恒星盘misalignment的样本，后期富坚补充HI的数据
2022/06/17
- 赵：利用高精度数值模拟构建不同时间不同半径处暗晕中的角动量分布函数（球壳坐标系）
- 以后讨论每两周一次，周一上午10点，下次讨论6月27日，富坚主讲半解析模型dark sage
链接
- 沈： size of galaxies File:Size.pdf