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- W1639268521 abstract "Abstract Three major modes of interaction in binary systems are identified, corresponding to (I) physical contact, (II) tidal mass loss from a star with a radiative envelope, and (III) tidal mass loss from a star with a convectlve envelope. The qualitative evolution of binary systems in each of these cases is outlined, leading to the formation of single white dwarfs, long-period remnants of quasi-conservative mass transfer, or short-period cataclysmic binaries. The origin of short-period double white dwarfs in a second phase of mass transfer is outlined. Implications for the frequency of different systems of these types, and of planetary nebulae with close binary nuclei, are discussed." @default.
- W1639268521 created "2016-06-24" @default.
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- W1639268521 date "1979-08-01" @default.
- W1639268521 modified "2023-09-23" @default.
- W1639268521 title "The Formation of White Dwarfs in Close Binary Systems" @default.
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- W1639268521 doi "https://doi.org/10.1017/s0252921100076338" @default.
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