Analysis of the subgiant halo star HD 76932

Details Analysis of the subgiant halo star HD 76932 Analysis of the subgiant halo star HD 76932

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....67..339b&link_type=abstract

Astronomy and Astrophysics, vol. 67, no. 3, July 1978, p. 339-344. Research supported by the Conselho Nacional de Pesquisas.

Astronomy and Astrophysics

Astrophysics

7

Atmospheric Composition, Late Stars, Stellar Atmospheres, Abundance, Atmospheric Models, Giant Stars, Kinematics, Stellar Spectra

Scientific paper

The chemical composition of the southern high-velocity star HD 76932 has been determined by means of a detailed analysis. The atmospheric model with a reciprocal effective temperature of 0.86 and log g = 3.5 was calculated by an interpolation in the grid of line-blanketed model atmospheres computed by Peytremann (1974). All the elements are found to be deficient by about the same factor of -1.1 dex with respect to the sun.

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