Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-24T17:47:29.942Z Has data issue: false hasContentIssue false
  • English
  • Français

Optically thick winds in novae

Published online by Cambridge University Press:  07 August 2017

Giora Shaviv
Giora Shaviv*
Affiliation:
Department of Physics, Asher Space Research Institute, and Miverva Center for Non-linear Physics, Israel Institute of Technology, Haifa, Israel, 32000

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.

We discuss the theory of optically thick winds from Novae, how they are treated numerically, and the effect of the mass loss on the long term evolution of the WD.

Keywords

stars: novaewhite dwarfswinds
Type
Session III - Anisotropic mass loss, disk formation
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 203 - 212
Copyright
Copyright © Kluwer 1995 

References

Bath, G.T., Shaviv, G. 1976, MNRAS 175, 305 CrossRefGoogle Scholar
Prialnik, D., Livio, M., Shaviv, G., Kovetz, A. 1982, ApJ 257, 312 CrossRefGoogle Scholar
Schwartzman, E., Kovetz, A., Prialnik, D. 1994, ApJ submitted Google Scholar