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Nearly 30,000 Late-type Main-sequence Stars with Stellar Age from LAMOST DR5
Zhang,Jiajun1,2; Zhao,Jingkun1; Oswalt,Terry D.3; Liang,Xilong1,2; Ye,Xianhao1,2; Zhao,Gang1,2
2021-02-01
Source PublicationThe Astrophysical Journal
ISSN0004-637X
Volume908Issue:2
AbstractAbstract We construct a sample of nearly 30,000 main-sequence stars with 4500 K?
KeywordStellar activity Stellar ages Stellar kinematics Late-type dwarf stars
DOI10.3847/1538-4357/abce5b
Language英语
WOS IDIOP:0004-637X-908-2-abce5b
PublisherThe American Astronomical Society
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Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/60571
Collection中国科学院国家天文台
Corresponding AuthorZhao,Jingkun
Affiliation1.CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China zjk@bao.ac.cn
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China
3.Embry-Riddle Aeronautical University, Aerospace Boulevard, Daytona Beach, FL 32114, USA; oswaltt1@erau.edu
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhang,Jiajun,Zhao,Jingkun,Oswalt,Terry D.,et al. Nearly 30,000 Late-type Main-sequence Stars with Stellar Age from LAMOST DR5[J]. The Astrophysical Journal,2021,908(2).
APA Zhang,Jiajun,Zhao,Jingkun,Oswalt,Terry D.,Liang,Xilong,Ye,Xianhao,&Zhao,Gang.(2021).Nearly 30,000 Late-type Main-sequence Stars with Stellar Age from LAMOST DR5.The Astrophysical Journal,908(2).
MLA Zhang,Jiajun,et al."Nearly 30,000 Late-type Main-sequence Stars with Stellar Age from LAMOST DR5".The Astrophysical Journal 908.2(2021).
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