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A non-local thermodynamic equilibrum study of scandium in the Sun
Zhang, H. W.1,2; Gehren, T.2; Zhao, G.3
2008-04-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume481Issue:2Pages:489-497
AbstractAims. We investigate the formation of neutral and singly ionized scandium lines in the solar photospheres. The research is aimed at derive solar log g f epsilon(circle dot)(Sc) values for scandium lines, which will later be used in differential abundance analyses of metal-poor stars.
KeywordLine : Formation Line : Profiles Sun : Abundances
DOI10.1051/0004-6361:20078910
Indexed BySCI
Language英语
WOS IDWOS:000254515800024
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8333
Collection光学天文研究部
Affiliation1.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
2.Univ Munich, Inst Astron & Astrophys, D-81679 Munich, Germany
3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Zhang, H. W.,Gehren, T.,Zhao, G.. A non-local thermodynamic equilibrum study of scandium in the Sun[J]. ASTRONOMY & ASTROPHYSICS,2008,481(2):489-497.
APA Zhang, H. W.,Gehren, T.,&Zhao, G..(2008).A non-local thermodynamic equilibrum study of scandium in the Sun.ASTRONOMY & ASTROPHYSICS,481(2),489-497.
MLA Zhang, H. W.,et al."A non-local thermodynamic equilibrum study of scandium in the Sun".ASTRONOMY & ASTROPHYSICS 481.2(2008):489-497.
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