Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..335b&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 2, Aug. 1991, p. 335-366. Research supported by DFG
Astronomy and Astrophysics
Astrophysics
105
Asymptotic Giant Branch Stars, Giant Stars, M Stars, Photosphere, Stellar Color, Supergiant Stars, Stellar Evolution, Stellar Models, Stellar Temperature, Stratification
Scientific paper
Colors and stratifications of a grid of spherically extended M giant and supergiant model photospheres described previously by Scholz (1985) have been supplemented and interpolated in metallicity, gravity, and photospheric extension so that they correspond to the parameter values of theoretical evolutionary supergiant branches for stars with masses of 1, 1.5, 2.25, 5, 10, and 15 solar masses and metallicities log Z/Z-solar of + 0.5, 0.0, - 0.3, - 0.6, and - 1.0. These colors may be used, for example, for comparison with observed supergiant branches or for synthesizing integrated spectra of clusters and galaxies.
Bessell Michael S.
Brett John M.
Scholz Marek
Wood Peter R.
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