Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T18:00:43.467Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of a 30 M⊙ star with mass loss

Published online by Cambridge University Press:  14 August 2015

H. J. Falk  and
R. Mitalas
H. J. Falk
Affiliation:
University of Western Ontario
R. Mitalas
Affiliation:
University of Western Ontario

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.

Evolutionary tracks for a 30 M⊙ star with mass loss rates (0.0, 1.0, 2.5, 5.0, 10.0)x10−7 M⊙/yr have been calculated. The effect of the different rates on the main sequence lifetime and on the effective temperature of the core He burning is discussed.

Type
Session 6: Evolution with Mass Loss: Single Stars
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 371 - 374
Copyright
Copyright © Reidel 1979 

References

Barbaro, G., Chiosi, C., and Nobili, L. 1971, Proceedings of the Trieste Colloquium on Supergiant Stars. Ed. Hack, M., p. 334.Google Scholar
Chiosi, C. and Nasi, E. 1974, Astron. Astrophys. 34, p. 355.Google Scholar
Chiosi, C., Nasi, E. and Sreenivasan, R. 1978, Astron. Astrophys. 63, p. 103.Google Scholar
de Loore, C., de Greve, J.P., Lamers, H.J.G.L.M. 1977, Astron. Astrophys. 61, p. 251.Google Scholar
Iben, I. 1966, Astrophys. J. 143, p. 516.CrossRefGoogle Scholar
McCrea, W. H. 1962, Astron. J. 71, p. 172.Google Scholar
Robertson, J. 1972, Astrophy. J. 177, p. 473.CrossRefGoogle Scholar
Simpson, E. 1971, Astrophys. J. 165, p. 295.CrossRefGoogle Scholar
Stothers, R. and Chin, C.-w. 1976, Astrophys. J. 204, p. 470.Google Scholar