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Evolution and nucleosynthesis of Wolf-Rayet stars

Published online by Cambridge University Press:  25 May 2016

Knut Jørgen Røed Ødegaard
Knut Jørgen Røed Ødegaard*
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, Blindern, N-0315 Oslo, Norway

Abstract

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Using a dynamical stellar code, detailed evolutionary models have been computed that follow the evolution and nucleosynthesis of massive stars from the pre-MS up through their most advanced stages.

Type
Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 256 - 257
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Langer, N. 1989, A&A 220, 135 Google Scholar
Ødegaard, K.J.R. 1996, in: Vreux, J.-M., Detal, A., Fraipont-Caro, D., Gosset, E. & Rauw, G. (eds.), Wolf-Rayet Stars in the Framework of Stellar Evolution, Proc. 33 rd Liège Int. Astroph. Coll. (Liège: Univ. of Liège), p. 81 Google Scholar
Ødegaard, K.J.R. 1997, in: Nota, A. & Lamers, H. (eds.), Luminous Blue Variables: Massive Stars in Transition, ASP-CS 120, 154 Google Scholar