Consulte o link da referência para acessar o original.
Sumário:
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.
Publicação:
Astronomy and Astrophysics, Vol. 67, p. 339-344 (1978)
Data da Publicação:
Julho de 1978
Referência:
