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Classical Novae as Super-Eddington Objects

Nir J. Shaviv
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Abstract

Several of the inconsistencies plaguing the field of novae are resolved once we consider novae to be steady state super-Eddington objects. In particular, we show that the super-Eddington shell burning state is a natural consequence of the equations of stellar structure, and that the predicted mass loss in the super-Eddington state agrees with nova observations. We also find that the transition phase of novae can be naturally explained as "stagnating" winds.

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Nir J. Shaviv. 2002-07-29. Classical Novae as Super-Eddington Objects. https://doi.org/10.1063/1.1518210

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