A Differential Abundance Analysis of HD219175A and B

Details A Differential Abundance Analysis of HD219175A and B A Differential Abundance Analysis of HD219175A and B

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chjaa...5..238z&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Volume 5, Issue 3, pp. 238-244 (2005).

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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