No CrossRef data available.
Article contents
Complete Stellar Models: Interior and Spectral Evolution of Massive Stars
Published online by Cambridge University Press: 07 August 2017
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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).
- Type
- Poster Papers
- Information
- Copyright
- Copyright © Kluwer 1995
References
Schaerer, D., de Koter, A., Schmutz, W., 1994, IAU Symp. 163, Eds. van der Hucht, K. A., Williams, P. M., Kluwer, Dordrecht, p. 300
Google Scholar