No CrossRef data available.
Article contents
The Origin and Evolution of Novae
Published online by Cambridge University Press: 12 April 2016
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 cataclysmic binaries are products of the nonconservative evolution of close binaries with large initial mass ratios of components. The accretors in cataclysmic binaries can be helium or carbon-oxygen or oxygen-neon-magnesium white dwarfs. Their annual birthrates are ~0.005, ~0.005, and ~0.00005 respectively. In one-zone approximation of a thin accreting shell we estimate the critical masses of hydrogen and helium shells and recurrence time scales of thermonuclear runaways.
- Type
- 3. Theory
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 325 - 341
- Copyright
- Copyright © Springer-Verlag 1990
References
Leising, M.D., 1987, In: Nucl. Spectr. Astrophys.Sources: Workshop, Washington, D.C., p.130.Google Scholar
Paczynski, B., 1976, in: Proc. IAU Symp. 73 “Structure and Evolution of Close Binary Stars”, p.75.
CrossRefGoogle Scholar
Ritter, H., Burkert, A., 1985, In: Recent Results on Cataclysmic Binaries, ESA SP-236.Google Scholar
Starrfield, S., Sparks, W.M., Truran, J.W., Kutter, G.S., 1972, Ap.J., 176, 169.CrossRefGoogle Scholar
Tutukov, A.V., Yungelson, L.R., 1979, In: Mass Loss and Evolution of O-Type Stars, Eds. Conti, P.S., De Loore, C., Reidel, Dordrecht, p.216,Google Scholar
Tutukov, A.V., Yungelson, L.R., 1985, In: Recent Results on Cataclysmic Variables, ESA SP-236, p.7.
Google Scholar
Tutukov, A.V., Fedorova, A.V., Ergma, E.V., Yungelson, L.R., 1985, Pisma Astron. Zh., 11, 123.Google Scholar
Tutukov, A.V., Fedorova, A.V., Ergma, E.V., Yungelson, L.R., 1987, Pisma Astron. Zh.
13, 780.Google Scholar
You have
Access