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- W2172061808 abstract "We show that the secondaries in short-period cata- clysmic variables with orbital periods P 3 hr, the earliest spectral types at a given period correspond to main sequence stars, while the majority of secondaries have later spectral types. Possible causes are nuclear evolution prior to mass transfer and lack of thermal equilibrium due to mass transfer. A comparison with evolutionary sequences obtained with up-to-date stellar mod- els implies unusually high transfer rates and a large fraction of systems with evolved donors. There is no evidence for a sec- ondary of low metallicity in any of the well-studied cataclysmic variables." @default.
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- W2172061808 date "1998-11-01" @default.
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- W2172061808 title "ARE THE RED DWARFS IN CATACLYSMIC VARIABLES MAIN-SEQUENCE STARS?" @default.
- W2172061808 hasPublicationYear "1998" @default.
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