The C and N abundances in disk stars
文献类型:期刊论文
作者 | Shi, JR![]() ![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
![]() |
出版日期 | 2002 |
卷号 | 381期号:3页码:982-992 |
关键词 | stars : abundances stars : late-type Galaxy : evolution Galaxy : solar neighbourhood |
英文摘要 | Abundance analysis of carbon and nitrogen has been performed for a sample of 90 F and G type main-sequence disk stars with a metallicity range of 1:0 < [Fe/H] < +0.2 using the C I and N I lines. We confirm a moderate carbon excess in the most metal-poor disk dwarfs found in previous investigations. Our results suggest that carbon is enriched by superwinds of metal-rich massive stars at the beginning of the disk evolution, while a significant amount of carbon is contributed by low-mass stars in the late stage. The observed behavior of [N/Fe] is about solar in the disk stars, irrespective of the metallicity. This result suggests that nitrogen is produced mostly by intermediate-mass stars. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000173458400033 |
源URL | [http://ir.bao.ac.cn/handle/114a11/8531] ![]() |
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.Peking Univ, Chinese Acad Sci, Joint Beijing Astrophys Ctr, Beijing 100871, Peoples R China |
推荐引用方式 GB/T 7714 | Shi, JR,Zhao, G,Chen, YQ. The C and N abundances in disk stars[J]. ASTRONOMY & ASTROPHYSICS,2002,381(3):982-992. |
APA | Shi, JR,Zhao, G,&Chen, YQ.(2002).The C and N abundances in disk stars.ASTRONOMY & ASTROPHYSICS,381(3),982-992. |
MLA | Shi, JR,et al."The C and N abundances in disk stars".ASTRONOMY & ASTROPHYSICS 381.3(2002):982-992. |
入库方式: OAI收割
来源:国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。