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Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
文献类型:期刊论文
作者 | Gehren, T; Shi, JR![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2006-06-01 |
卷号 | 451期号:3页码:1065-1079 |
关键词 | line : formation line : profiles stars : abundances stars : late-type Galaxy : evolution |
英文摘要 | Aims. Parameters for 55 nearby metal-poor stars are determined using high-resolution spectroscopy. Together with similar data taken from a recent analysis, they are used to show trends of their Galactic evolution with stellar [Fe/H] or [Mg/H] abundances. The separation of abundance ratios between disk and halo stars is used as a basic criterion for population membership. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000237329000045 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7109] ![]() |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Univ Munich, Inst Astron & Astrophys, D-81679 Munich, Germany 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 3.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 4.Uppsala Astron Observ, S-75120 Uppsala, Sweden |
推荐引用方式 GB/T 7714 | Gehren, T,Shi, JR,Zhang, HW,et al. Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars[J]. ASTRONOMY & ASTROPHYSICS,2006,451(3):1065-1079. |
APA | Gehren, T,Shi, JR,Zhang, HW,Zhao, G,&Korn, AJ.(2006).Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars.ASTRONOMY & ASTROPHYSICS,451(3),1065-1079. |
MLA | Gehren, T,et al."Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars".ASTRONOMY & ASTROPHYSICS 451.3(2006):1065-1079. |
入库方式: OAI收割
来源:国家天文台
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