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Numerical Modelling of the Classical Nova Outburst
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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- Copyright © Springer-Verlag 1988