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Complete Stellar Models: Interior and Spectral Evolution of Massive Stars

Published online by Cambridge University Press:  07 August 2017

D. Schaerer ,
A. De Koter  and
W. Schmutz
D. Schaerer
Affiliation:
Geneva Observatory, CH-1290 Sauverny, Switzerland
A. De Koter
Affiliation:
NASA/GSCF USRA, Greenbelt, MD 20771, USA
W. Schmutz
Affiliation:
Institut für Astronomie, ETH Zurich, CH-8092 Zürich, Switzerland

Extract

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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).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 363
Copyright
Copyright © Kluwer 1995 

References

de Koter, A., Schmutz, W., Lamers, H.J.G.L.M., 1993, A&A 277, 561 Google Scholar
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
Schaerer, D., Schmutz, W., 1994a, A&A 288, 231 Google Scholar