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Numerical Modelling of the Classical Nova Outburst

Published online by Cambridge University Press:  12 April 2016

G. Siegfried Kutter  and
Warren M. Sparks
G. Siegfried Kutter
Affiliation:
Lab. for Astronomy and Solar Physics, NASA/Goddard Space Flight Center
Warren M. Sparks
Affiliation:
Applied Theoretical Physics Division, Los Alamos National Laboratory

Abstract

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We describe a mechanism that promises to explain how classical nova outbursts take place on white dwarfs of 1 M⊙ or less and for accretion rates of 4 × 10−10 M⊙ yr−1 or greater.

Type
Part III. Chemical and Dynamical Structures of Exploding Stars
Information
International Astronomical Union Colloquium , Volume 108: Atmospherics Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion , 1988 , pp. 236 - 237
Copyright
Copyright © Springer-Verlag 1988

References

Bibliography:

Kutter, G.S., and Sparks, W.M. 1980, Ap. J., 239, 988.Google Scholar
Kutter, G.S., and Sparks, W.M. 1987, Ap. J., 321, 386.Google Scholar
Livio, M., and Shara, M.M. 1987, Ap. J., 319, 819.Google Scholar
Patterson, J. 1984, Ap. J. Suppl., 54, 443.CrossRefGoogle Scholar
Prialnik, D., and Kovetz, A. 1984, Ap. J., 281, 367.Google Scholar
Sparks, W.M., and Kutter, G.S. 1987, Ap. J., 321, 394.Google Scholar
Starrfield, S., Sparks, W.M., and Truran, J.W. 1985, Ap. J., 291, 136.CrossRefGoogle Scholar