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- W147330918 abstract "We present the basic properties of symbiotic novae, and show how they differ from classical novae. Differences are observationally particularly noticeable in the luminosity curve, the rise of which is much slower, but its return to pre-outburst level takes much longer than in classical novae. Special emphasis is given to the intial phase, for which two different evolutionary paths have been observed. The outburst may lead into a supergiant phase lasting for several years, which is being followed by the nebular phase, or it may lead straight into the nebular phase. The total energy radiated during an outburst is at least as large as the energy loss of classical novae. Mass-loss during outburst may be sufficiently small to lead eventually to a supernova on the white dwarf." @default.
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- W147330918 date "1992-01-01" @default.
- W147330918 modified "2023-09-26" @default.
- W147330918 title "The Outburst of Symbiotic Novae" @default.
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- W147330918 doi "https://doi.org/10.1017/s0074180900122648" @default.
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