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VW Hyi: A Rapidly Cooling White Dwarf?
Published online by Cambridge University Press: 12 April 2016
Abstract
We 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.
- Type
- Space Observations
- Information
- International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 251 - 252
- Copyright
- Copyright © Kluwer 1996