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- W2054500713 abstract "Understanding boundary layer heating is crucial in determining the thermal structure of the accreted envelope of a prenova white dwarf. The matched asymptotic expansion method was used to solve consistently for the structure of accretion disks transferring matter onto rotating white dwarfs. The fraction of accretion energy transported into prenova white dwarf envelopes was calculated. These results should be used by modelers of nova eruptions; they will produce significantly lower degeneracies and weaker explosions than expected until now. Detailed models of accretion disks and boundary layers can also be used to calculate the amount of white dwarf heating during a dwarf nova outburst. In general, such models can serve as input to model atmosphere codes to predict more realistic spectra of disk-accreting objects. 29 refs." @default.
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- W2054500713 date "1989-05-01" @default.
- W2054500713 modified "2023-09-27" @default.
- W2054500713 title "How much boundary layer heating occurs in an accreting prenova white dwarf?" @default.
- W2054500713 doi "https://doi.org/10.1086/167453" @default.
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