A high-resolution spectral analysis of mildly metal-poor stars II. Chemical abundances
文献类型：期刊论文
| 作者 | Qiu, HM; Zhao, G ; Zhong, JY
|
| 刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2003 |
| 卷号 | 27期号:1页码:66-72 |
| 关键词 | star : abundance star : atmosphere star : individuals : HD22484, HD51530, HD59984 |
| 英文摘要 | On the basis of a previous paper, we have determined the atmospheric parameters and the abundance of nine chemical elements for a sample of stars. we discuss the changes of the abundances with [Fe/H]. The mean [Na/Fe]similar to-0.01 dex is close to the solar abundance. Of the alpha elements Si and Ca possess almost the same abundance model, [Ti/Fe] has a rather large scatter while all three tend to increase with decreasing [Fe/H]. The iron-peak elements V, Cr and Ni have comparatively large scatters in their abundance. For all the sample stars, [Cr/Fe] is over-abundant, and [Mn/Fe] is under-abundant. The latter also increases with increasing metal abundances. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000181305100007 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8441]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Qiu, HM,Zhao, G,Zhong, JY. A high-resolution spectral analysis of mildly metal-poor stars II. Chemical abundances[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2003,27(1):66-72. |
| APA | Qiu, HM,Zhao, G,&Zhong, JY.(2003).A high-resolution spectral analysis of mildly metal-poor stars II. Chemical abundances.CHINESE ASTRONOMY AND ASTROPHYSICS,27(1),66-72. |
| MLA | Qiu, HM,et al."A high-resolution spectral analysis of mildly metal-poor stars II. Chemical abundances".CHINESE ASTRONOMY AND ASTROPHYSICS 27.1(2003):66-72. |
入库方式： OAI收割
来源：国家天文台
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