Models of stellar evolution and their use in calibrating distances and element abundances of stars

Details Models of stellar evolution and their use in calibrating distances and element abundances of stars Models of stellar evolution and their use in calibrating distances and element abundances of stars

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...109..187g&link_type=abstract

Astronomy and Astrophysics, vol. 109, no. 1, May 1982, p. 187-190.

Astronomy and Astrophysics

Astrophysics

10

Abundance, Star Clusters, Stellar Evolution, Stellar Parallax, Calibrating, Solar Temperature, Stellar Interiors, Stellar Luminosity, Stellar Models

Scientific paper

Recently published grids of stellar interior models fail to account for
the temperature and luminosity of the Sun with reasonable values of
mass, age and chemical composition. It is shown how this discrepancy may
affect the determination of element abundances and distances of field
stars and clusters.

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