A Differential Abundance Analysis of HD219175A and B

Hua-Wei Zhang, Gang Zhao

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, 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.

Keywords


stars: abundances --- stars: atmospheres --- binaries: visual

Full Text:

PDF


DOI: http://dx.doi.org/10.1088/1009-9271%2F5%2F3%2F003

Refbacks

  • There are currently no refbacks.



Print ISSN: 1674-4527

Online ISSN: 2397-6209