中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Spectrometric composition of nearby K dwarfs

文献类型:期刊论文

作者Kotoneva, E.; Shi, J. R.; Zhao, G.; Liu, Y. J.
刊名ASTRONOMY & ASTROPHYSICS
出版日期2006-08-01
卷号454期号:3页码:833-U77
关键词stars : abundances stars : low mass, brown dwarfs Galaxy : solar neighbourhood
英文摘要We have obtained relatively high resolution spectra of Northern hemisphere K dwarfs. This is the first spectrometric project dedicated only to K dwarfs. Earlier studies have concentrated on more massive F and G dwarfs. However, these stars have already undergone evolutionary effects, unlike K dwarfs, which over more accurate information about the evolution of the Solar neighbourhood. We have determined the LTE abundances of 14 elements for 42 stars with initial metallicity range covered by -1.52 < [Fe/H] < 0.48. We confirm the discrepancy in the abundances derived from neutral and ionized lines. The solution to this problem cannot just be the modification of initial physical parameters, but requires fundamental changes in the modeling of K dwarfs.
收录类别SCI
语种英语
WOS记录号WOS:000239121200021
源URL[http://ir.bao.ac.cn/handle/114a11/7203]  
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.Turku Univ, Piikkio, Finland
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Kotoneva, E.,Shi, J. R.,Zhao, G.,et al. Spectrometric composition of nearby K dwarfs[J]. ASTRONOMY & ASTROPHYSICS,2006,454(3):833-U77.
APA Kotoneva, E.,Shi, J. R.,Zhao, G.,&Liu, Y. J..(2006).Spectrometric composition of nearby K dwarfs.ASTRONOMY & ASTROPHYSICS,454(3),833-U77.
MLA Kotoneva, E.,et al."Spectrometric composition of nearby K dwarfs".ASTRONOMY & ASTROPHYSICS 454.3(2006):833-U77.

入库方式: OAI收割

来源:国家天文台

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