Abstract
We present the first models of massive stars, where the interior structure is coupled to a spherically extended, metal line blanketed non-LTE atmosphere with a wind. This is accomplished with the Geneva stellar evolution code and the non-LTE atmosphere code of de Koter et al. (1993). The method described in Schaerer & Schmutz (1994) is used to treat line blanketing. A first account of this work is published in Schaerer et al. (1994).
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References
de Koter A., Schmutz W., Lamers H.J.G.L.M., 1993, A&A 277, 561.
Schaerer D., de Koter A., Schmutz W., 1994, IAU Syrnp. 163, Eds. K.A. van der Hucht, P.M. Williams, Kluwer, Dordrecht, p. 300.
Schaerer D., Schmutz W., 1994a, A&A 288, 231.
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© 1995 Springer Science+Business Media Dordrecht
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Schaerer, D., De Koter, A., Schmutz, W. (1995). Complete Stellar Models: Interior and Spectral Evolution of Massive Stars. In: van der Kruit, P.C., Gilmore, G. (eds) Stellar Populations. International Astronomical Union / Union Astronomique Internationale, vol 164. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0125-7_39
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DOI: https://doi.org/10.1007/978-94-011-0125-7_39
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