中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Abundance analysis of mildly metal-poor stars

文献类型:期刊论文

作者Qiu, HM; Zhao, G; Xin, Y; Li, ZW
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期2001
卷号25期号:1页码:65-72
关键词metal-poor stars element abundances
英文摘要We present here some observed data on 11 mildly metal-poor stars with -1.3 less than or equal to [Fe/H] less than or equal to -0.6. The model parameters and the abundances of 14 elements are determined. We also discuss the relation between the abundance ratio and the metallicity. The or elements (Mg, Si, Ca, Ti) are overabundant relative to Fe with a varying scatter at each given metallicity. Most of the iron-peak elements (V, Cr, Ni, Cu) are also overabundant relative to Fe by amounts that are independent of [Fe/H], while [Mn/Fe] increases with increasing metallicity. [Na/Al] is overabundant in the sample with [Fe/H]> -1.1 and definitely overdeficient in the sample with [Fe/H]< -1.1.
收录类别SCI
语种英语
WOS记录号WOS:000167510400009
源URL[http://ir.bao.ac.cn/handle/114a11/8626]  
专题国家天文台_太阳物理研究部
作者单位1.Chinese Acad Sci, Beijing Astron Observ, Beijing 100012, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
推荐引用方式
GB/T 7714
Qiu, HM,Zhao, G,Xin, Y,et al. Abundance analysis of mildly metal-poor stars[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2001,25(1):65-72.
APA Qiu, HM,Zhao, G,Xin, Y,&Li, ZW.(2001).Abundance analysis of mildly metal-poor stars.CHINESE ASTRONOMY AND ASTROPHYSICS,25(1),65-72.
MLA Qiu, HM,et al."Abundance analysis of mildly metal-poor stars".CHINESE ASTRONOMY AND ASTROPHYSICS 25.1(2001):65-72.

入库方式: OAI收割

来源:国家天文台

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