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- W2085804533 abstract "view Abstract Citations (35) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Gravitational radiation and the evolution of cataclysmic binaries. Taam, R. E. ; Flannery, B. P. ; Faulkner, J. Abstract Results are presented for several evolutionary sequences of close binary systems which resemble dwarf novae. The systems, containing white dwarfs and main-sequence companions, have masses less than 3.4 solar masses and periods less than 17 hours. The loss of angular momentum by gravitational radiation is included in the calculations. It is found that a system can be captured as a result of evolution dominated by gravitational radiation losses when the primary encounters its Roche lobe while near the main sequence. In such a case, the system evolves to even shorter periods, with the nuclear time scale of the primary increasing so that the latter is unable to exhaust hydrogen. Other sequences do not result in capture (1) when the primary is sufficiently evolved that it can exhaust hydrogen during mass exchange and (2) when a simple model for mass and angular momentum losses associated with nova outbursts from the accreting white dwarf is considered Publication: The Astrophysical Journal Pub Date: August 1980 DOI: 10.1086/158190 Bibcode: 1980ApJ...239.1017T Keywords: Binary Stars; Gravitational Waves; Stellar Evolution; Variable Stars; Angular Momentum; Dwarf Stars; Hydrogen; Novae; Stellar Mass Ejection; Astrophysics full text sources ADS | data products SIMBAD (5)" @default.
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- W2085804533 date "1980-08-01" @default.
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- W2085804533 title "Gravitational radiation and the evolution of cataclysmic binaries" @default.
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