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- W3006060445 abstract "The eruption of a (classical) nova is widely accepted to be a recurrent event in the lifetime of a cataclysmic binary star. In-between eruptions the system should therefore behave as a normal cataclysmic variable (CV), i.e. according to its characteristic properties like the mass-transfer rate or the strength of the magnetic field of the white dwarf. How important are these characteristics for the nova eruption itself, i.e. which type of systems preferably undergo a nova eruption? This question could in principle be addressed by comparing the post-nova systems with the general CV population. However, information on post-novae is scarce, even to the extent that the identification of the post-nova is ambiguous in most cases. In this paper we inform on the progress of a project that has been undertaken to significantly improve the number of confirmed post-novae, thus ultimately providing the means for a better understanding of these objects." @default.
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- W3006060445 date "2013-01-01" @default.
- W3006060445 modified "2023-09-23" @default.
- W3006060445 title "Getting to Know the Cataclysmic Variable Beneath the Nova Eruption" @default.
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