| 报告主题 |
报告人 |
时间 |
地点 |
| Modifying BSE algorithm to realize sdB star evolution |
Xiaogang Wang （王小刚） |
Dec. 08, 2022 |
Room 427 of Main Building |
| Disk dissipation and giant planet formation in the past three-million-year history of Gould’s Belt |
Mingchao LIU（刘明超） |
Dec. 08, 2022 |
Room 427 of Main Building |
| Derivative spectrosocpy and its applications in sky survey |
Lihuan YU（于立欢） |
Dec. 01, 2022 |
Room 427 of Main Building |
| Surface helium abundance of hot subdwarfs considering gravitational settling and radiative levitation |
Ruijie JI（吉瑞杰） |
Dec. 01, 2022 |
Room 427 of Main Building |
| The difference in efficiencies between low-mass and high-mass common envelopes |
Yingzhen CUI（崔英朕） |
Dec. 01, 2022 |
Room 427 of Main Building |
| Analysis of triple spectra from the LAMOST-MRS survey |
Tongyu HE（何同禹） |
Nov. 24, 2022 |
Room 427 of Main Building |
| Identify main-sequence binaries from Chinese Space Station Telescope photometric system using machine learning |
Jiajia LI（李佳佳) |
Nov. 24, 2022 |
Room 427 of Main Building |
| The Modification and Improvement of Measuring Stellar Parameters by Machine Learning |
Jiarui RAO（饶加睿） |
Nov. 17, 2022 |
Room 427 of Main Building |
| Modelling mass transfer in binary systems |
Jingqi CHEN（陈静琦） |
Nov. 17, 2022 |
Room 427 of Main Building |
| Mass and Age Determination of the LAMOST Data with Different Machine Learning Methods |
Qida LI（李启达） |
Nov. 17, 2022 |
Room 427 of Main Building |
| The Radius of Accreting Main Sequence Stars |
Ziqi ZHAO（赵梓琪） |
Nov. 10, 2022 |
Room 427 of Main Building |
| Common envelope candidates and parameters determination |
Qiyuan CHENG（程其原) |
Nov. 10, 2022 |
Room 427 of Main Building |
| Search for accreting neutron star binary candidates using Chinese Space Station Telescope |
Hao SHEN（申灏） |
Nov. 10, 2022 |
Room 427 of Main Building |
| The population of hot subdwarf stars studied with LAMOST |
Jiangdan LI（李江丹） |
Nov. 03, 2022 |
Room 427 of Main Building |
| The progenitors of SNe Ia with AGB donors |
Luhan LI（李陆翰) |
Nov. 03, 2022 |
Room 427 of Main Building |
| Formation of Be binaries through He star channel |
Yuchen BAO（鲍昱辰） |
Nov. 03, 2022 |
Room 427 of Main Building |
| Irradiation driven mass-transfer cycles in LMXBs |
Shunyi LAN（兰顺义） |
Oct.27,2022 |
Room 427 of Main Building |
| 3D hydrodynamical simulations of type Ia supernova remnants: influence of a binary companion star |
Jingxiao LUO（罗竞霄） |
Oct.27,2022 |
Room 427 of Main Building |
| Formation of Be binaries through He star channel |
Yuchen BAO（鲍昱辰） |
Oct. 27, 2022 |
Room 427 of Main Building |
| The hydrodynamical simulations of accreting WDs with high accretion rates |
Yingzhen CUI（崔英朕） |
April 15, 2021 |
Room 427 of Main Building |
