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- W3100658181 abstract "The evolution of the soft X-ray emission of V1974 Cyg has been simulated by a white dwarf envelope model with steady hydrogen burning. The comparison of the results obtained from ROSAT observations with the results of our envelope models indicates that the post-outburst evolution of the nova can be explained by steady H-burning on either a 0.9 white dwarf with 50% degree of mixing between solar-like accreted material and the ONe degenerate core, or on a 1.0 ONe white dwarf with 25% mixing." @default.
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- W3100658181 date "2005-08-12" @default.
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- W3100658181 title "Envelope models for the supersoft X-ray emission of V1974 Cyg" @default.
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- W3100658181 doi "https://doi.org/10.1051/0004-6361:20042587" @default.
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