Hostname: page-component-8448b6f56d-xtgtn Total loading time: 0 Render date: 2024-04-19T05:34:43.042Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Masses of the White Dwarfs in Classical Nova Systems

Published online by Cambridge University Press:  12 April 2016

James W. Truran  and
Mario Livio
James W. Truran
Affiliation:
University of Illinois
Mario Livio
Affiliation:
Department of Physics, Technion

Extract

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.

Significant progress in our understanding of the nature of the outbursts of the classical novae has occurred over the past two decades (see, e.g., reviews by Truran 1982; Starrfield 1986). Their outbursts are now understood to be driven by thermonuclear runaways proceeding in the accreted hydrogen-rich shells on the white dwarf components of close binary systems. Critical parameters which serve to dictate the varied characteristics of the observed outbursts include the intrinsic white dwarf luminosity, the rate of mass accretion, the composition of the envelope matter prior to runaway, and the white dwarf mass.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 114: White Dwarfs , 1989 , pp. 498 - 506
Copyright
Copyright © Springer-Verlag 1989

References

Anders, E., and Eibhara, M. 1982, Geochim. Cosmochim. Acta., 46, 2363.Google Scholar
Bath, G.T., and Shaviv, G. 1978, M.N.R.A.S., 183, 515 Google Scholar
Cameron, A.G.W. 1982, in Essays In Nuclear Astrophysics, ed. Barnes, C.A., Clayton, D.D., and Schramm, D.N. (Cambridge: Cambridge University Press), p. 23.Google Scholar
Collin-Souffrin, S. 1977, in Novae and Related Stars. ed. Friedjung, M. (Dordrecht: Reidel), p. 123.Google Scholar
Duerbeck, H.W. 1984, AstroPhys. Space Sci., 99, 363 Google Scholar
Ferland, G.J. 1979, Ap. J., 231, 781.Google Scholar
Ferland, G.J., and Shields, G.A. 1978, Ap. J., 226, 172 Google Scholar
Fujimoto, M. 1982, Ap. J., 257, 752 Google Scholar
Gallagher, J.S., Hege, E.K., Kopriva, D.A., Williams, R.E., and Butcher, H.R. 1980, Ap. J., 237, 55 Google Scholar
Haefner, R., and Metz, K. 1985, Astr. Ap., 145, 311.Google Scholar
Hameury, J.-M., King, A.R., Lasota, J.-P., and Livio, M. 1988, submitted to M.N.R.A.S.Google Scholar
Koester, D., Schulz, H., and Weidemann, V. 1979, Astr. Ap., 76, 262 Google Scholar
Kovetz, A., and Prialnik, D. 1985, Ap. J., 291, 812 Google Scholar
Law, W.Y., and Ritter, H. 1983, Astr. Ap., 123, 33 Google Scholar
Livio, M. 1988, in IAU Colloq. 108, Atmospheric Diagnostics of Stellar Evolution. ed. Nomoto, K., in press.Google Scholar
Livio, M., and Truran, J.W. 1987, Ap. J., 318, 316 Google Scholar
MacDonald, J. 1983, Ap. J., 267, 732 Google Scholar
Pacheco, J.A.F. 1977, M.N.R.A.S., 181, 421.Google Scholar
Paczynski, B. 1971, Acta. Astr., 21, 417 Google Scholar
Patterson, J. 1984, Ap. J. Suppl., 54, 443.Google Scholar
Payne-Gaposchkin, C.. 1957, The Galactic Novae. (Amsterdam: North Holland).Google Scholar
Politano, M.J. and Webbink, R.F. 1988, poster paper this conference.Google Scholar
Prialnik, D., Livio, M., Shaviv, G. andKovetz, A. 1982, Ap. J., 257, 312 Google Scholar
Salpeter, E.E. 1955, Ap. J., 121, 161 Google Scholar
Snijders, M.A.J., Batt, T.J., Seaton, M.J., Blades, J.C., and Morton, D.C.. 1984, M.N.R.A.S., 211, 7P.Google Scholar
Starrfield, S. 1986, preprint.Google Scholar
Starrfield, S., Sparks, W.M. and Truran, J.W. 1985, Ap. J., 219, 136 CrossRefGoogle Scholar
Stickland, D.J., Penn, C.J., Seaton, M.J., Snijders, M.A.J., and Storey, P.J. 1981, M.N.R.A.S., 197, 107 CrossRefGoogle Scholar
Truran, J.W. 1982, in Essays in Nuclear Astrophysics, ed. Barnes, C.A., Clayton, D.D., and Schramm, D.N. (Cambridge: Cambridge University Press), p. 467.Google Scholar
Truran, J.W. 1985a, in Production and Distribution of CNO Elements, ed. Danziger, I.J. (Garching: ESO), p. 211.Google Scholar
Truran, J.W. 1985b, in Nucleosynthesis: Challenges and New Developments, ed. Arnett, W.D., and Truran, J.W. (Chicago: University of Chicago Press), p. 292. Google Scholar
Truran, J.W., and Livio, M. 1986, Ap. J., 308, 721.Google Scholar
Truran, J.W., Shankar, A., Livio, M., and Hayes, J. 1988, in preparation.Google Scholar
Tylenda, R. 1978, Acta. Astr., 28, 333 Google Scholar
Williams, R.E. 1985, in Production and Distribution of CNO Elements. ed. Danziger, I.J. (Garching: ESO), p. 225. Google Scholar
Williams, R.E., and Gallagher, J.S. 1979, Ap. J., 228, 482 Google Scholar
Williams, R.E., Sparks, W.M., Starrfield, S., Ney, E.P., Truran, J.W., and Wyckoff, S. 1985, M.N.R.A.S., 212, 753 Google Scholar
Williams, R.E., Woolf, N.J., Hege, E.K., Moore, R.L., and Kopriva, D.A. 1978, Ap. J., 224, 171 CrossRefGoogle Scholar
Woosley, S.E. 1987, in Nucleosynthesis and Chemical Evolution, eds. Hauck, E., Maeder, A., and Meynet, G. (Geneva: Geneva Observatory), p. 82.Google Scholar