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A Differential Abundance Analysis of HD219175 A and B
作者姓名:Hua-Wei  Zhang  and  Gang  Zhao
作者单位:Hua-Wei Zhang and Gang Zhao Department of Astronomy,School of Physics,Peking University,Beijing 100871; National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012
基金项目:Supported by the National Natural Science Foundation of China.
摘    要:The 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.

关 键 词:微分丰度  HD  219175恒星          光谱观测

A Differential Abundance Analysis of HD219175 A and B
Hua-Wei Zhang and Gang Zhao.A Differential Abundance Analysis of HD219175 A and B[J].Chinese Journal of Astronomy and Astrophysics,2005,5(3):238-244.
Authors:Hua-WeiZhang GangZhao
Institution:[1]DepartmentofAstronomy,SchoolofPhysics,PekingUniversity,Beijing100871 [2]NationalAstronomicalObservatories,ChineseAcademyofSciences,Beijing100012
Abstract:The 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, A1, 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.
Keywords:stars: abundances - stars: atmospheres - binaries: visual
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