Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-20T03:21:47.997Z Has data issue: false hasContentIssue false
  • English
  • Français

Chemical evolution and mixing processes in massive stars

Published online by Cambridge University Press:  07 August 2017

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

Abstract

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.

The first results of new evolutionary calculations of massive stars are presented. The calculations cover ZAMS masses from 20—200 M⊙. Yields and abundances throughout the stars are presented.

Keywords

stars: massive starsevolutionnucleosynthesismixing
Type
Session V - poster summaries
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 322 - 323
Copyright
Copyright © Kluwer 1995 

References

Caughlan, G.R., Fowler, W.A. 1988, Atomic Data and Nuclear Data Tables, 40, 283 Google Scholar
Fuller, G.M., Fowler, W.A., Newman, M.J. 1982, ApJ Suppl. 48, 279 CrossRefGoogle Scholar
Itoh, N., Adachi, T., Nakagawa, M., Kohyama, Y. 1989, ApJ 339, 354 Google Scholar
Itoh, N., Mutoh, H., Hikita, A. 1992, ApJ 395, 622 Google Scholar
Langer, N., Eid, M. E., Fricke, K. 1985, A&A 145, 179 Google Scholar
Thielemann, F.-K., Arnould, M, Truran, J.W. 1987, in: Hillebrandt, W., Kuhfuß, R., Müller, E. & Truran, (eds.), Lecture Notes in Physics: Nuclear Astrophysics, Vol. 287, p. 233 Google Scholar
Wagenhuber, J., Weiss, A. 1994, A&A submitted Google Scholar