No CrossRef data available.
Article contents
The effects of boundary conditions on stellar evolution
Published online by Cambridge University Press: 04 August 2017
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 effects of using different treatments of the surface boundary conditions are investigated in the context of the mass of He White Dwarfs. We find that since the White Dwarf progenitor is a star with a very extended atmosphere, the results are sensitive to the degree of accuracy implemented in the handling of the boundary conditions.
- Type
- Mass Loss from Hot Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 463 - 464
- Copyright
- Copyright © Reidel 1987
References
Reimers, D., 1975, “Problems in Stellar Atmospheres and Envelopes”, p.229, Ed. Baschek, B., Keggel, W. H., Tremaine, G., Springer, Berlin, Heidelberg, New York.Google Scholar
Van den Berg, D.A., Hartwick, F.D.A., Dawson, P., Alexander, D.R., 1983, Ap. J.
266, 747.Google Scholar
You have
Access