中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler

文献类型:期刊论文

作者Wu, Ya-Qian1; Xiang, Mao-Sheng2; Zhang, Xian-Fei1; Li, Tan-Da2; Bi, Shao-Lan1; Liu, Xiao-Wei3; Fu, Jian-Ning1; Huang, Yang3; Tian, Zhi-Jia3; Liu, Kang1
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2017
卷号17期号:1
关键词stars: fundamental parameters stars: evolution stars: asteroseismology
英文摘要Main sequence turn-off (MSTO) stars have advantages as indicators of Galactic evolution since their ages can be robustly estimated from atmospheric panuneters. Hundreds of thousands of MSTO stars have been selected from the LAMOST Galactic survey to study the evolution of the Galaxy, and it is vital to derive accurate stellar parameters. In this work, we select 150 MSTO star candidates from the MSTO star sample of Xiang that have asteroseismic parameters and determine accurate stellar parameters for these stars by combining asteroseismic parameters deduced froth Kepler photometry and atmospheric parameters deduced from LAMOST spectra. With this simple, we examine the age determination as well as the contamination rate of the MSTO star sample. A comparison of age between this work and Xiang shows a mean difference of 0.53 Gyr (7%) and a dispersion of 2.71 Gyr (28%). The results show that 79 of the candidates are MSTO stars, while the others are contaminations from either main sequence or sub-giant stars. The contamination rate for the oldest stars is much higher than that for younger stars. The main cause for the high contamination rate is found to be the relatively large systematic bias in the LAMOST surface gravity estimates.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]SOLAR-LIKE OSCILLATIONS ; 1ST DATA RELEASE ; RED GIANTS ; ELEMENT DIFFUSION ; EVOLUTION ; ASTEROSEISMOLOGY ; METALLICITY ; ROTATION ; CLUSTERS ; TEMPERATURE
收录类别SCI
语种英语
WOS记录号WOS:000396489000005
源URL[http://ir.bao.ac.cn/handle/114a11/8260]  
专题国家天文台_太阳物理研究部
作者单位1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714
Wu, Ya-Qian,Xiang, Mao-Sheng,Zhang, Xian-Fei,et al. Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2017,17(1).
APA Wu, Ya-Qian.,Xiang, Mao-Sheng.,Zhang, Xian-Fei.,Li, Tan-Da.,Bi, Shao-Lan.,...&Li Tanda.(2017).Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,17(1).
MLA Wu, Ya-Qian,et al."Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 17.1(2017).

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。