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High-resolution Spectroscopic Analysis of a Large Sample of Li-rich Giants Found By LAMOST
Zhou,Yutao1,2; Yan,Hongliang1,2; Shi,Jianrong1,2; Blanco-Cuaresma,S.3; Gao,Qi1,2; Pan,K.4; Xu,Xiaodong1,2; Zhang,Junbo1; Zhao,Gang1,2
刊名The Astrophysical Journal
2019-05-31
卷号877期号:2
关键词stars: abundances stars: chemically peculiar stars: evolution stars: late-type
ISSN号0004-637X
DOI10.3847/1538-4357/ab1b4b
英文摘要Abstract The discovery of Li-rich giants has introduced a new challenge for standard stellar evolution models. To resolve this issue, the number of this type of object has been rapidly increased through the development of worldwide surveys. Taking advantage of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope survey, 44 new Li-rich giants are reported, which are confirmed with high-resolution observations. Based on the high-resolution and high signal-to-noise spectra, we derived the atmospheric parameters and elemental abundances with the spectral synthesis method. We performed a detailed analysis of their evolutionary stages, infrared excess, projected rotational velocity ( ), and stellar population. We find that (1) the Li-rich giants concentrate at the evolutionary status of the red giant branch bump, red clump, and asymptotic giant branch; (2) three of them are fast rotators and none exhibit infrared excess. Our results imply that the origins of Li enrichment are most likely to be associated with the extra mixing in the stellar interior, and the external sources might only make a minor contribution. Moreover, various Li-rich episodes take place at different evolutionary stages.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-877-2-AB1B4B
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/26421]  
专题中国科学院国家天文台
作者单位1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China zhouyutao@nao.cas.cn, sjr@nao.cas.cn
2.University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China
3.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
4.Apache Point Observatory and New Mexico State University, P.O. Box 59, Sunspot, NM, 88349-0059, USA
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GB/T 7714
Zhou,Yutao,Yan,Hongliang,Shi,Jianrong,et al. High-resolution Spectroscopic Analysis of a Large Sample of Li-rich Giants Found By LAMOST[J]. The Astrophysical Journal,2019,877(2).
APA Zhou,Yutao.,Yan,Hongliang.,Shi,Jianrong.,Blanco-Cuaresma,S..,Gao,Qi.,...&Zhao,Gang.(2019).High-resolution Spectroscopic Analysis of a Large Sample of Li-rich Giants Found By LAMOST.The Astrophysical Journal,877(2).
MLA Zhou,Yutao,et al."High-resolution Spectroscopic Analysis of a Large Sample of Li-rich Giants Found By LAMOST".The Astrophysical Journal 877.2(2019).
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