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- W17168967 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." @default.
- W17168967 created "2016-06-24" @default.
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- W17168967 date "1996-01-01" @default.
- W17168967 modified "2023-09-25" @default.
- W17168967 title "VW Hyi: A Rapidly Cooling White Dwarf?" @default.
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- W17168967 doi "https://doi.org/10.1007/978-94-009-0325-8_75" @default.
- W17168967 hasPublicationYear "1996" @default.
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