Author:
Gänsicke Boris T.,Beuermann Klaus
Abstract
AbstractWe estimate the post-outburst cooling time-scale of the white dwarf in VW Hyi, using the available quiescent IUE spectra. The determination of the white-dwarf temperature close to the outburst is hampered because disc emission still contributes to the SWP flux.
Publisher
Cambridge University Press (CUP)