Hostname: page-component-7b7567c8c-fvjsw Total loading time: 0 Render date: 2026-11-15T22:48:26.397Z Has data issue: false hasContentIssue false
  • English
  • Français

Classical Nova Evolution: Clues from Soft X-Ray Emission

Published online by Cambridge University Press:  12 April 2016

James MacDonald
James MacDonald*
Affiliation:
University of Delaware, Department of Physics and Astronomy, Newark, DE 19716, 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.

Multi-wavelength observations have shown that, after optical decline, the stellar remnants of classical nova outbursts evolve at constant, near-Eddington, bolometric luminosity to high effective temperature (> 2 105 K), before turning off. Here we briefly review the observations of classical novae in this phase of evolution, and discuss what the soft X-ray observations tell us about the mass of the underlying white dwarf and the rate of mass change due to stellar winds and accretion from the stellar companion.

Information

Type
Novae & Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996, pp. 281 - 287
Copyright
Copyright © Kluwer 1996

References

Bath, G.T., 1978, MNRAS, 182, 35 CrossRefGoogle Scholar
Bowyer, S., Lieu, R., Lampton, M., et al., 1994, Ap. J. Supp., 93, 569 CrossRefGoogle Scholar
Feast, M.W., Glass, I.S., 1974, MNRAS, 167, 81 CrossRefGoogle Scholar
Fujimoto, M.Y., Iben, I., 1992, AJ, 399, 646 CrossRefGoogle Scholar
Gallagher, J.S., Code, A.D., 1974, Ap. J., 189, 303 CrossRefGoogle Scholar
Gallagher, J.S., Starrfield, S., 1976, MNRAS, 176, 3 Google Scholar
Gallagher, J.S., Starrfield, S., 1978, ARAA, 16, 171 CrossRefGoogle Scholar
Geisel, S.L., Kleinmann, D.E., Low, F.J., 1970, Ap. J., 161, L101 CrossRefGoogle Scholar
Hyland, A.R., Neugebauer, G., 1970, Ap. J., 160, L177 CrossRefGoogle Scholar
Kato, M., 1983, PASJ, 35, 507 Google Scholar
Kato, M., Hachisu, I., 1994, Ap. J., 437, 802 CrossRefGoogle Scholar
Krautter, J., Ögelman, H., Starrfield, S., 1992, IAUC 5550 Google Scholar
Krautter, J., Starrfield, S., 1995, private communicationGoogle Scholar
Krautter, J., Williams, R.E., 1989, Ap. J., 341, 968 CrossRefGoogle Scholar
Kurtz, D.W., Vanden Bout, P.A., Angel, J.R.P., 1972, Ap. J., 178, 701 CrossRefGoogle Scholar
Lloyd, H.M., O’Brien, T.J., Bode, M.F., et al., 1992, Nature, 356, 222 CrossRefGoogle Scholar
MacDonald, J., 1980, MNRAS, 191, 933 Google Scholar
MacDonald, J., 1983, Ap. J., 267, 732 CrossRefGoogle Scholar
MacDonald, J., 1984, Ap. J., 283, 241 Google Scholar
MacDonald, J., Fujimoto, M.Y., Truran, J.W., 1985, Ap. J., 294, 263 CrossRefGoogle Scholar
MacDonald, J., Vennes, S., 1991, Ap. J., 373, L51 CrossRefGoogle Scholar
MacDonald, J., Vennes, S., 1994, AAS meeting Minneapolis, MN, May 29 – June 2Google Scholar
Mason, K.O., Cordova, F.A., Bode, M.F., Ban, P., 1987, in “RS Ophiuchi (1985) and the Recurrent Nova Phenomenon”, ed. Bode, M.F., VNU Science Press, Utrecht, p 167 Google Scholar
O’Brien, T., Kahn, F.D., Bode, M.F., 1987, in “RS Ophiuchi (1985) and the Recurrent Nova Phenomenon”, ed. Bode, M.F., VNU Science Press, Utrecht, p 177 Google Scholar
Ögelman, H., Beuermann, K., Krautter, J., 1984, Ap. J., 287, L31 CrossRefGoogle Scholar
Ögelman, H., Krautter, J., Beuermann, K., 1987, A&A, 177, 110 Google Scholar
Ögelman, H., Orio, M., Krautter, J., Starrfield, S., 1993, Nature, 361, 331 CrossRefGoogle Scholar
Paresce, F., Livio, M., Hack, W., Korista, K., 1995, A&A, 299, 823 Google Scholar
Pequignot, D., 1996, these proceedings, p305Google Scholar
Prialnik, D., Shara, M., 1995, AJ, 109, 1735 CrossRefGoogle Scholar
Prialnik, D., Kovetz, A., 1995, Ap. J., 445, 789 CrossRefGoogle Scholar
Shanley, L., Ögelman, H., Gallagher, J.S., et al., 1995, Ap. J., 438, L95 CrossRefGoogle Scholar
Starrfield, S., 1979, in “White Dwarfs and Variable Degenerate Stars”, ed. Van Horn, H.M. and Weidemann, V., p 274 Google Scholar
Starrfield, S., Truran, J.W., Sparks, W.M., Kutter, G.S., 1974, Ap. J., 176, 169 CrossRefGoogle Scholar
Starrfield, S., Shore, S.N., Sparks, W.M., et al., 1992, Ap. J., 391, L71 CrossRefGoogle Scholar
Starrfield, S., et al., 1996, in IAU Colloquium 152, “Astrophysics in the Extreme Ultraviolet”, Cambridge University Press, Cambridge, in pressGoogle Scholar
Stringfellow, S.G., Bowyer, S., 1994, in “Interacting Binary Stars”, ed. Shatter, A., ASP Conf. Ser. 56, 315 Google Scholar
Warner, B., 1990 in IAU Colloquium 122, “Physics of Classical Novae”, eds Cassatella, A., Viotti, R., Springer-Verlag, Berlin, p24 Google Scholar