Stellar physics and population in the open cluster lab

中国科学院云南天文台学术报告通知

2025年第7

报告题目Stellar physics and population in the open cluster lab

报告人Xiaoting FU(符晓婷)

报告人单位中国科学院紫金山天文台

报告语言:中文或英文

报告时间43日(星期四)14:30-15:30

报告地点1号楼412会议室

报告摘要

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Open clusters provide an ideal laboratory for testing and calibrating our understanding of stellar physics and single stellar population. In this talk, I will discuss how astronomers use open clusters as a well-defined single population of stars to study the Milky Way disk and stellar evolution. Additionally, I will explore how open clusters can be used to validate pipeline results from large photometric and spectroscopic surveys, ensuring that we obtain reliable measurements of stellar properties.

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报告人简介:

Dr. Xiaoting Fu is an associate research professor at the Purple Mountain Observatory, Chinese Academy of Sciences. After receiving her Ph.D. degree in 2016 from the International School for Advanced Studies (SISSA) in Trieste, Italy. Xiaoting worked in the University of Bologna and then the Kavli Institute for Astronomy and Astrophysics (KIAA) as a PostDoc. Xiaoting is mainly working on stars, both theoretically and observationally, including stellar modelling, stellar chemical abundances, stellar clusters, and using stars to study the Galactic chemical evolution. Xiaoting is the science co-leader of the MSE (MaunaKea Spectroscopic Explorer) Milky Way working group, and is an active member of several large surveys, such as the Gaia-ESO Survey, Chinese Space Station Telescope (CSST), and MUltiplexed Survey Telescope (MUST).


邀请人:柳正伟、陈雪飞

邀请方:大样本恒星演化研究团组、国际超新星中心、国际超新星研究重点实验室




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