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- W4231542376 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)." @default.
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- W4231542376 date "1995-01-01" @default.
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- W4231542376 title "Complete Stellar Models: Interior and Spectral Evolution of Massive Stars" @default.
- W4231542376 doi "https://doi.org/10.1017/s0074180900108824" @default.
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