中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Chemical abundances of 10 metal-poor halo stars

文献类型:期刊论文

作者Bai, GS; Zhao, G; Chen, YQ; Shi, JR; Klochkova, VG; Panchuk, VE; Qiu, HM; Zhang, HW
刊名ASTRONOMY & ASTROPHYSICS
出版日期2004-10-01
卷号425期号:2页码:671-681
关键词stars : abundances stars : fundamental parameters Galaxy : abundances Galaxy : halo
英文摘要We present observations of ten metal-poor halo stars with the metallicity range -2.3<[Fe/H]<-1.4 and derive their stellar parameters, acquire some elemental abundances relative to iron and discuss the relation between the abundance ratio and the metallicity. It was found that oxygen abundances are nearly constant at a level of 0.6 dex for our metal-poor halo stars when the non-LTE correction is considered. The alpha-elements (Mg, Si, Ca and Ti) are overabundant relative to Fe and decrease with increasing metallicity. We also obtained a significant underabundant non-LTE [Na/Fe] ratio from Na I D lines which have a large deviation from the LTE assumption. Scandium is marginally overabundant with respect to iron and tends to decrease with increasing metallicity like the alpha-elements. A nearly solar value of [Cr/Fe] ratio and underabundant [Mn/Fe] ratio are obtained.
收录类别SCI
语种英语
WOS记录号WOS:000224526500027
源URL[http://ir.bao.ac.cn/handle/114a11/6938]  
专题国家天文台_光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
3.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714
Bai, GS,Zhao, G,Chen, YQ,et al. Chemical abundances of 10 metal-poor halo stars[J]. ASTRONOMY & ASTROPHYSICS,2004,425(2):671-681.
APA Bai, GS.,Zhao, G.,Chen, YQ.,Shi, JR.,Klochkova, VG.,...&Zhang, HW.(2004).Chemical abundances of 10 metal-poor halo stars.ASTRONOMY & ASTROPHYSICS,425(2),671-681.
MLA Bai, GS,et al."Chemical abundances of 10 metal-poor halo stars".ASTRONOMY & ASTROPHYSICS 425.2(2004):671-681.

入库方式: OAI收割

来源:国家天文台

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