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1995•Symposium - International Astronomical UnionOpen access

Complete Stellar Models: Interior and Spectral Evolution of Massive Stars

D. Schaerer, A. De Koter, W. Schmütz

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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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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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Available 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).

Key concepts: Blanketing, Stellar atmosphere, Stars, Physics, Atmosphere (unit), Stellar evolution, Astrophysics, Astronomy

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