中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5

文献类型:期刊论文

作者Luo,Yangping2; Németh,Péter1,3; Deng,Licai2,4; Han,Zhanwen5
刊名The Astrophysical Journal
出版日期2019-08-06
卷号881期号:1
关键词stars: kinematics and dynamics subdwarfs surveys
ISSN号0004-637X
DOI10.3847/1538-4357/ab298d
英文摘要Abstract Combing Gaia DR2 with LAMOST DR5, we spectroscopically identified 924 hot subdwarf stars, among which 32 stars exhibit strong double-lined composite spectra. We measured the effective temperature Teff, surface gravity , helium abundance y?=?nHe/nH, and radial velocities (RVs) of 892 non-composite spectra hot subdwarf stars by fitting LAMOST observations with Tlusty/Synspec non-LTE synthetic spectra. We outlined four different groups in the diagram with our helium abundance classification scheme and two nearly parallel sequences in the diagram. 3D Galactic space motions and orbits of 747 hot subdwarf stars with (GBP???GRP)0?
语种英语
WOS记录号IOP:0004-637X-881-1-AB298D
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/27417]  
专题中国科学院国家天文台
作者单位1.Astroserver.org, 8533 Malomsok, Hungary
2.Department of Astronomy, China West Normal University, Nanchong, 637002, People’s Republic of China; ypluo@bao.ac.cn
3.Astronomical Institute of the Czech Academy of Sciences, CZ-25165, Ondr?ejov, Czech Republic
4.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, People’s Republic of China
推荐引用方式
GB/T 7714
Luo,Yangping,Németh,Péter,Deng,Licai,et al. Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5[J]. The Astrophysical Journal,2019,881(1).
APA Luo,Yangping,Németh,Péter,Deng,Licai,&Han,Zhanwen.(2019).Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5.The Astrophysical Journal,881(1).
MLA Luo,Yangping,et al."Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5".The Astrophysical Journal 881.1(2019).

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