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Thermonuclear Runaway Models for Symbiotic Novae
Published online by Cambridge University Press: 12 April 2016
Abstract
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This paper reviews the basic physics of thermonuclear runaways on the surfaces of accreting white dwarf stars, with a special emphasis on understanding the evolution of symbiotic novae.
- Type
- Session 2. The Physics of the Symbiotic Phenomenon
- Information
- International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 161 - 168
- Copyright
- Copyright © Kluwer 1988
References
Shustov, B.M., and Tutukov, A.V.
1985. Recent Results on Cataclysmic Variables (ESA SP-236), p. 113.Google Scholar
Sion, E.M., and Starrfield, S.G.
1985. in Recent Results on Cataclysmic Variables (ESA SP-236), p. 17.Google Scholar
Tutukov, A.V. and Yungeľson, L.R.
1982. in IAU Colloquium No. 70, The Nature of Symbiotic Stars, ed. Friedjung, M. and Viotti, R. (Dordrecht: Reidel), p. 283.Google Scholar