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Lithium evolution in the low-mass evolved stars with asteroseismology and LAMOST spectroscopy

Hong-Liang Yan Gang Zhao Jing-Hua Zhang Yu-Tao Zhou Qi Gao Jian-Rong Shi Yerra Bharat Kumar Wako Aoki Haining Li Chunqian Li

自然科学基础研究(英文)Issue(4):1547-1555,9.
自然科学基础研究(英文)Issue(4):1547-1555,9.DOI:10.1016/j.fmre.2023.08.005

Lithium evolution in the low-mass evolved stars with asteroseismology and LAMOST spectroscopy

Lithium evolution in the low-mass evolved stars with asteroseismology and LAMOST spectroscopy

Hong-Liang Yan 1Gang Zhao 2Jing-Hua Zhang 3Yu-Tao Zhou 4Qi Gao 3Jian-Rong Shi 2Yerra Bharat Kumar 5Wako Aoki 6Haining Li 3Chunqian Li2

作者信息

  • 1. CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Beijing 100101,China||Institute for Frontiers in Astronomy and Astrophysics,Beijing Normal University,Beijing 102206,China||School of Astronomy and Space Science,University of Chinese Academy of Sciences,Beijing 100049,China
  • 2. CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Beijing 100101,China||School of Astronomy and Space Science,University of Chinese Academy of Sciences,Beijing 100049,China
  • 3. CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Beijing 100101,China
  • 4. College of Mathematics and Physics,Guangxi Minzu University,Nanning 530006,China||Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China||Department of Astronomy,School of Physics,Peking University,Beijing 100871,China
  • 5. CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Beijing 100101,China||Indian Institute of Astrophysics,100ft road Koramangala,Bangalore,560034,India
  • 6. National Astronomical Observatory of Japan,Tokyo 181-8588,Japan||Department of Astronomical Science,School of Physical Sciences,The Graduate University for Advanced Studies(SOKENDAI),Tokyo 181-8588,Japan
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摘要

关键词

Stellar evolution/Stellar abundances/Lithium stars/Chemically peculiar stars/Red giant stars/Red giant clump/Low-mass star/Asteroseismology

Key words

Stellar evolution/Stellar abundances/Lithium stars/Chemically peculiar stars/Red giant stars/Red giant clump/Low-mass star/Asteroseismology

引用本文复制引用

Hong-Liang Yan,Gang Zhao,Jing-Hua Zhang,Yu-Tao Zhou,Qi Gao,Jian-Rong Shi,Yerra Bharat Kumar,Wako Aoki,Haining Li,Chunqian Li..Lithium evolution in the low-mass evolved stars with asteroseismology and LAMOST spectroscopy[J].自然科学基础研究(英文),2025,(4):1547-1555,9.

基金项目

This work is supported by the National Natural Science Founda-tion of China(11988101,12090040,12090044,12022304,11833006,11973052,11973049,11890694,and U2031203),the National Key R&D Program of China(2019YFA0405502).We acknowledge the sup-port of the JSPS-CAS Joint Research Program.H.-L.Y.and H.L.acknowledge support from the Youth Innovation Promotion Associa-tion of the CAS(id.2019060 and Y202017,respectively),and NAOC Nebula Talents Program.J.-H.Z.acknowledges support from NSFC(12103063)and from China Postdoctoral Science Foundation funded project(2020M680672).Y.B.K acknowledges the support of the NSFC(11850410437).H.L.acknowledges support from the Strategic Priority Research Program of Chinese Academy of Sciences,(XDB34020205).Guoshoujing Telescope(the Large Sky Area Multi-Object Fiber Spectro-scopic Telescope,LAMOST)is a National Major Scientific Project built by the Chinese Academy of Sciences.Funding for the project has been provided by the National Development and Reform Commission.LAM-OST is operated and managed by the National Astronomical Observato-ries,Chinese Academy of Sciences. (11988101,12090040,12090044,12022304,11833006,11973052,11973049,11890694,and U2031203)

自然科学基础研究(英文)

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