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个人简介
I obtained my PhD degree from the Department of Astronomy of Beijing Normal University. I have a position of assistant research fellow at Xinjiang Astronomical Observatory, Chinese Academy of Sciences . I am interested in variable stars, especially the asteroseismology of pulsating stars in open clusters. The open clusters can be a good "probe" of the nature of the Milky Way, and can also provide a key constraint on the structure and evolution of the Milky Way. By identification of members of pulsating stars and asteroseismology analysis, especially the one in binary systems, one can obtain the stellar parameters independently and test the formation and evolution of stars. We can further study the nature of the clusters, such as size, age, mass, metal abundance, binary fraction, formation, dynamical evolution and etc.
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Jayanand Maurya, M. R. Samal, Louis Amard, Yu Zhang,Hubiao Niu, Sang Chul Kim, Y. C. Joshi, B. Kumar
arxiv(2024)
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Kexue tongbaono. 21 (2023): 2790-2804
The Astrophysical Journalno. 2 (2022): 80-80
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