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adifferentialabundanceanalysisofhd219175aandb
Zhang Huawei1; Zhao Gang2
2005
Source Publicationchinesejournalofastronomyandastrophysics
ISSN1009-9271
Volume5Issue:3Pages:238
AbstractThe abundances of the wide binary pair HD 219175 A and B are determined and compared using a line-by-line differential analysis. No evidence for difference has been found in the abundances of Fe, O, Na, Mg, Al, Si, K, Ca, Sc, Ti, V, Cr, Mn, Ni, Cu and Ba. Our results support a physical relation between the two components of HD 219175.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/45080
Collection中国科学院国家天文台
Affiliation1.北京大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
Zhang Huawei,Zhao Gang. adifferentialabundanceanalysisofhd219175aandb[J]. chinesejournalofastronomyandastrophysics,2005,5(3):238.
APA Zhang Huawei,&Zhao Gang.(2005).adifferentialabundanceanalysisofhd219175aandb.chinesejournalofastronomyandastrophysics,5(3),238.
MLA Zhang Huawei,et al."adifferentialabundanceanalysisofhd219175aandb".chinesejournalofastronomyandastrophysics 5.3(2005):238.
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