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- W2125767194 abstract "Evolutionary changes of masses and periods under the influence of gravitational radiation (GR) are computed for binaries with main-sequence or degenerate hydrogen-helium (H), helium (He) and carbon (C) secondaries. Tracks in the P-M 2 and P-M 2 planes are determined. The orbital period of systems P with a non-degenerate dwarf filling its Roche lobe decreases until the time-scale of GR (~ 10 9 −10 10 yrs) becomes shorter than the thermal time-scale τ KH of the mass losing component M 2 . When M 2 becomes ~ 0.1 M ⊙ , P begins to increase. This could account for the existence of the minimal P ≈ 1.3 h and for the accumulation of observed cataclysmic binaries (CB) below P ≤ 2 h . The GR can be the driving force for evolution of cataclysmic binaries: TT Ari, OY Car, Z Cha, and WZ Sge as their P , M 2 and indicate. The rate of mass exchange driven by GR is ~ 10 −9 −10 −10 M ⊙ /yrs. It is enough to feed the X-ray bursters and related objects." @default.
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- W2125767194 date "1981-01-01" @default.
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- W2125767194 title "Evolution of Low Mass Binaries under the Influence of Gravitational Radiation" @default.
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- W2125767194 doi "https://doi.org/10.1017/s0074180900073903" @default.
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