Lithium abundances of nearby young solar-type stars based on optical high-resolution spectroscopy
文献类型：期刊论文
| 作者 | Xing, L. -F.1; Xing, Q. -F.2 |
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2012 |
| 卷号 | 537 |
| 关键词 | stars: evolution stars: abundances stars: solar-type |
| 英文摘要 | Context. Lithium has long been recognized as a powerful tool for investigating the internal mixing of low-mass stars. In addition, accurate measurements of lithium abundances in young solar-type stars provide independent and reliable age diagnostics. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000300416800091 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6240]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Zhengzhou Univ Light Ind, Dept Technol & Phys, Zhengzhou 45002, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Xing, L. -F.,Xing, Q. -F.. Lithium abundances of nearby young solar-type stars based on optical high-resolution spectroscopy[J]. ASTRONOMY & ASTROPHYSICS,2012,537. |
| APA | Xing, L. -F.,&Xing, Q. -F..(2012).Lithium abundances of nearby young solar-type stars based on optical high-resolution spectroscopy.ASTRONOMY & ASTROPHYSICS,537. |
| MLA | Xing, L. -F.,et al."Lithium abundances of nearby young solar-type stars based on optical high-resolution spectroscopy".ASTRONOMY & ASTROPHYSICS 537(2012). |
入库方式： OAI收割
来源：国家天文台
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