Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-29T19:12:32.787Z Has data issue: false hasContentIssue false
  • English
  • Français

Thick winds from Wolf-Rayet stars

Published online by Cambridge University Press:  07 August 2017

D. Eichler ,
A. Bar Shalom  and
Y. Oreg
D. Eichler
Affiliation:
Department of Physics, Ben Gurion University, Beer Sheva, Israel
A. Bar Shalom
Affiliation:
Department of Physics, Ben Gurion University, Beer Sheva, Israel
Y. Oreg
Affiliation:
Department of Physics, Ben Gurion University, Beer Sheva, Israel

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.

When the effective opacity becomes sufficiently great, a qualitatively different type of radiatively driven wind solution appears, in which a high wind thickness and trapping of radiation cause each other in a bootstrap fashion. It is proposed that the thick winds from Wolf-Rayet stars can be understood in this manner. Opacity computations using the method of super transition arrays (STA) are presented that show that outflows from WR stars can attain the needed opacities.

Type
Session II - Model atmospheres for single Wolf-Rayet stars
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 172 - 173
Copyright
Copyright © Kluwer 1995 

References

Bar Shalom, A. Oreg, J. Goldstein, W.H., Shvarts, D., Zigler, A. 1989, Phys. Rev. A 40, 3183 CrossRefGoogle Scholar
de Silva, L.B. et al. 1992, Phys. Rev. Lett. 69, 438 CrossRefGoogle Scholar
Igelsias, C.A., Rogers, F.J. 1990, in : Goldstein, W.H., Hooper, C., Ganthier, J., Seely, J., Lee, R. (eds.), OPAL Opacities for Astrophysical Applications, Proc. 4th Int. Workshop on Radiative Properties of Hot Dense Matter (Singapore: World Scientific), p. 196 Google Scholar