| 报告主题 |
报告人 |
时间 |
地点 |
| The radius variations of accreting main-sequence stars and mass transfer instability |
ZHAO Ziqi(赵梓琪) |
9 May 2024 |
Room 412 of the main building |
| Recent discovery of Gaia BH3 |
KOVALEV Mikhail |
9 May 2024 |
Room 412 of the main building |
| He-accreting oxygen-neon white dwarfs and accretion-induced collapse events |
ZHANG Zhengyang(张正阳) |
25 Apr 2024 |
Room 412 of the main building |
| The evolution and final outcome for helium stars |
ZHANG Lifu(张力夫) |
25 Apr 2024 |
Room 412 of the main building |
| Measure distances based on periodic variable stars |
CHEN Xiaodian(陈孝钿) |
25 Apr 2024 |
Room 412 of the main building |
| Derivative Spectroscopy and its application at LAMOST-MRS |
YU Lihuan(于立欢) |
18 Apr 2024 |
Room 412 of the main building |
| Early excess emission in Type Ia supernovae: the interaction between supernova ejecta and circumstellar material |
XIAO Yu(肖雨) |
18 Apr 2024 |
Room 412 of the main building |
| Determination method of binary fractions by the integrated spectrum |
ZHANG Fenghui(张奉辉) |
18 Apr 2024 |
Room 412 of the main building |
| Detected false positive SB2 in LAMOST-MRS data attributable to the moonlight |
WANG Zhoulin(王洲林) |
11 Apr 2024 |
Room 412 of the main building |
| The completeness of accreting neutron star binary candidates from Chinese Space Station Telescope |
SHEN Hao(申灏) |
11 Apr 2024 |
Room 412 of the main building |
| LAMOST meets Gaia DR3: Explore Open Cluster metallicity trend and migration |
ZHANG Ruyuan(张汝媛) |
11 Apr 2024 |
Room 412 of the main building |
| Estimating the Atmospheric Parameters of Early-type Stars from CSST Slitless Spectra Survey |
RAO Jiarui(饶加睿) |
18 Jan 2024 |
Room 412 of the main building |
| Using CSST and ejecta-wind interaction in Type II-P supernovae to constrain the wind mass loss of red supergiant stars |
LUO Jingxiao(罗竞霄) |
18 Jan 2024 |
Room 412 of the main building |
| Mass-gap Black Hole Formation in Core-collapse supernovae |
ZHA Shuai(查帅) |
18 Jan 2024 |
Room 412 of the main building |
| The Formation of the Stripped-envelope Type IIb Supernova Progenitors: Rotation, Metallicity, and Overshooting |
LONG Gang(龙刚) |
11 Jan 2024 |
Room 412 of the main building |
| Does the inclination angle effect of the disk dominate IR SED slope (α) distribution ? |
LIU Mingchao(刘明超) |
11 Jan 2024 |
Room 412 of the main building |
| A He-CEW model for SN 2020eyj |
MENG Xiangcun(孟祥存) |
11 Jan 2024 |
Room 412 of the main building |
| Luminosity, Mass and Age of Early-Type Stars from LAMOST Survey |
LI Qida(李启达) |
04 Jan 2024 |
Room 412 of the main building |
| Ultraluminous X-Ray Sources with Helium star companions |
LI Luhan(李陆翰) |
04 Jan 2024 |
Room 412 of the main building |
| The influence of metallicity on the relative rate of stripped-envelope to Type II supernovae |
LIU Zhengwei(柳正伟) |
04 Jan 2024 |
Room 412 of the main building |
