中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Rotating Halo Traced by the K-giant Stars from LAMOST and Gaia

文献类型:期刊论文

作者Tian,Hao; Liu,Chao; Xu,Yan; Xue,Xiangxiang
刊名The Astrophysical Journal
出版日期2019-01-30
卷号871期号:2
ISSN号0004-637X
关键词galaxies: individual (Milky Way) Galaxy: halo Galaxy: kinematics and dynamics
DOI10.3847/1538-4357/aaf6e8
英文摘要Abstract With the help of Gaia DR2, we are able to obtain the full 6D phase space information for stars from the Large Sky Area Multi-Object Fibre Spectroscopic Telescope DR5. With high precision of the position, velocity, and metallicity, the rotation of the local stellar halo is presented using the K-giant stars with [Fe/H]?
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-871-2-AAF6E8
源URL[http://ir.bao.ac.cn/handle/114a11/24984]  
专题中国科学院国家天文台
作者单位Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Datun Road 20A, Beijing 100012, People’s Republic of China; liuchao@nao.cas.cn
推荐引用方式
GB/T 7714
Tian,Hao,Liu,Chao,Xu,Yan,et al. Rotating Halo Traced by the K-giant Stars from LAMOST and Gaia[J]. The Astrophysical Journal,2019,871(2).
APA Tian,Hao,Liu,Chao,Xu,Yan,&Xue,Xiangxiang.(2019).Rotating Halo Traced by the K-giant Stars from LAMOST and Gaia.The Astrophysical Journal,871(2).
MLA Tian,Hao,et al."Rotating Halo Traced by the K-giant Stars from LAMOST and Gaia".The Astrophysical Journal 871.2(2019).

入库方式: OAI收割

来源:国家天文台

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