High-degree Nonradial Pulsations in Fast-Rotating, Eclipsing Binary and Exoplanet Host Stars

中国科学院云南天文台学术报告通知

2025年第48

报告题目High-degree Nonradial Pulsations in Fast-Rotating, Eclipsing Binary and Exoplanet Host Stars

报告人:Prof. David Mkrtichian

报告人单位:National Astronomical Research Institute of Thailand (NARIT)

报告语言:English

报告时间:2025910日(星期三)14:30-15:30

报告地点:科研1号楼523会议室

报告摘要:

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I will discuss the primary challenge of practical asteroseismology—the difficulties in detecting and identifying high-degree, non-radial, small-scale modes and outline methods for overcoming this issue. I will report on the results of my spectroscopic survey of the search for and study of non-radial pulsations in bright, rapidly rotating A-type stars, pulsating components of eclipsing binaries, and stars with exoplanets.

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报告人简介:

David is a globally recognized authority expert in studying pulsating mass-accreting components in semi-detached eclipsing binary systems, particularly the oscillating Eclipsing Algol (oEA) stars - a class he originally discovered and classified. He has worked in several international astronomical organizations, including the National Astronomical Research Institute of Thailand (NARIT), the Astrophysical Research Center for Structure and Evolution of Cosmos (Sejong University, South Korea), the Crimean Astrophysical Observatory (Ukraine), and the Astronomical Observatory of Odessa National University (Ukraine). He has led or organized numerous international research and projects, including photometric and spectroscopic observations of pulsating stars, asteroseismology, exoplanets, and more.

云台邀请方:双星与变星研究团组

邀请方联系人:朱俐颖 




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