中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Detecting the Sagittarius Stream with LAMOST DR4 M Giants and Gaia DR2

文献类型:期刊论文

作者Li,Jing2,3; Liu,Chao4; Xue,Xiangxiang4; Zhong,Jing3; Weiss,Jake1; Carlin,Jeffrey L.5; Tian,Hao4
刊名The Astrophysical Journal
出版日期2019-04-01
卷号874期号:2
ISSN号0004-637X
关键词galaxies: individual (Sagittarius dSph) Galaxy: halo Galaxy: structure stars: abundances stars: distances stars: late-type
DOI10.3847/1538-4357/ab09ef
英文摘要Abstract We use LAMOST DR4 M giants combined with Gaia DR2 proper motions and ALLWISE photometry to obtain an extremely pure sample of Sagittarius (Sgr) stream stars. Using TiO5 and CaH spectral indices as indicators, we selected a large sample of M-giant stars from M-dwarf stars in LAMOST DR4 spectra. Considering the position, distance, proper motion, and angular momentum distribution, we obtained 164 pure Sgr stream stars. We find that the trailing arm has higher energy than the leading arm in the same angular momentum. The trailing arm we detected extends to a heliocentric distance of ~130 kpc at Λ ? ⊙ ~ 170 ° , which is consistent with the feature found in RR Lyrae in Sesar et al. Both of these detections of Sgr, in M-giants and in RR Lyrae, imply that the Sgr stream may contain multiple stellar populations with a broad metallicity range.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-874-2-AB09EF
源URL[http://ir.bao.ac.cn/handle/114a11/25657]  
专题中国科学院国家天文台
作者单位1.Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, 110 Eighth Street, Troy, NY 12180, USA
2.Physics and Space Science College,China West Normal University, 1 ShiDa Road, Nanchong 637002, People’s Republic of China; lijing@shao.ac.cn
3.SHAO, Chinese Academy of Sciences, Nandan Road, Shanghai 200030, People’s Republic of China
4.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Datun Road 20A, Beijing 100012, People’s Republic of China
5.LSST, 950 North Cherry Avenue, Tucson, AZ 85719, USA
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GB/T 7714
Li,Jing,Liu,Chao,Xue,Xiangxiang,et al. Detecting the Sagittarius Stream with LAMOST DR4 M Giants and Gaia DR2[J]. The Astrophysical Journal,2019,874(2).
APA Li,Jing.,Liu,Chao.,Xue,Xiangxiang.,Zhong,Jing.,Weiss,Jake.,...&Tian,Hao.(2019).Detecting the Sagittarius Stream with LAMOST DR4 M Giants and Gaia DR2.The Astrophysical Journal,874(2).
MLA Li,Jing,et al."Detecting the Sagittarius Stream with LAMOST DR4 M Giants and Gaia DR2".The Astrophysical Journal 874.2(2019).

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来源:国家天文台

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