Hostname: page-component-84b7d79bbc-dwq4g Total loading time: 0 Render date: 2024-07-30T04:46:37.733Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermonuclear Runaway Models for Symbiotic Novae

Published online by Cambridge University Press:  12 April 2016

Scott J. Kenyon
Scott J. Kenyon*
Affiliation:
Smithsonian Astrophysical Observatory Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138, USA

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.

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

Fujimoto, M.Y. 1982a. Astrophys. J., 257, 752.CrossRefGoogle Scholar
Fujimoto, M.Y. 1982b. Astrophys. J., 257, 767.CrossRefGoogle Scholar
Gallagher, J.S. and Starrfield, S.G. 1978. Ann. Rev. Astr. Astrophys., 16, 171.Google Scholar
Iben, I. Jr. 1982. Astrophys. J., 259, 244.Google Scholar
Iben, I. Jr. and Renzini, A. 1983. Ann. Rev. Astr. Astrophys., 21, 271.Google Scholar
Kenyon, S.J. and Truran, J.W. 1983. Astrophys. J., 273, 280.CrossRefGoogle Scholar
Kenyon, S.J. and Webbink, R.F. 1984. Astrophys. J., 279, 252.Google Scholar
Kutter, G.S. and Sparks, W.M. 1980. Astrophys. J., 239, 988.CrossRefGoogle Scholar
MacDonald, J. 1980. Mon. Not. Roy. Astr. Soc., 191, 933.CrossRefGoogle Scholar
MacDonald, J. 1983. Astrophys. J., 267, 732.CrossRefGoogle Scholar
Nariai, K., Nomoto, K., and Sugimoto, D. 1980. Pub. Astr. Soc. Japan,, 32, 472.Google Scholar
Paczyński, B. 1970. Acta Astr., 21, 417.Google Scholar
Paczyński, B. and Rudak, B. 1980. Astr. Astrophys., 82, 349.Google Scholar
Paczyński, B. and Żytkow, A. 1978. Astrophys. J., 222, 604.Google Scholar
Prialnik, D. 1986. Astrophys. J., 310, 222.CrossRefGoogle Scholar
Prialnik, D., Livio, M., Shaviv, G., and Kovetz, A. 1982. Astrophys. J., 257, 312.Google Scholar
Shustov, B.M., and Tutukov, A.V. 1985. Recent Results on Cataclysmic Variables (ESA SP-236), p. 113.Google Scholar
Sion, E.M., Ademo, M.J., and Tomczyk, S. 1979. Astrophys. J., 232, 832.Google Scholar
Sion, E.M., and Starrfield, S.G. 1985. in Recent Results on Cataclysmic Variables (ESA SP-236), p. 17.Google Scholar
Starrfield, S., Sparks, W.M., and Truran, J.W. 1984, Astrophys. J., 291, 136.Google Scholar
Tutukov, A.V. and Yungeľson, L.R. 1976. Astrofizika, 12, n21.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
Uus, U. 1970. Nauk Informatsii, 17, 32.Google Scholar