Evolution of low-mass close binaries with orbital angular momentum losses

Details Evolution of low-mass close binaries with orbital angular momentum losses Evolution of low-mass close binaries with orbital angular momentum losses

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24...85t&link_type=abstract

(Astrofizika, vol. 24, Jan.-Feb. 1986, p. 85-96) Astrophysics (ISSN 0571-7132), vol. 24, no. 1, July 1986, p. 51-59. Translation

Statistics

Computation

13

Angular Momentum, Binary Stars, Cataclysmic Variables, Stellar Evolution, Stellar Mass Ejection, Stellar Orbits, Computational Astrophysics, Stellar Gravitation, Stellar Magnetic Fields, Stellar Mass Accretion, Stellar Winds

Scientific paper

The evolution of secondary components in close binary systems with compact primary components is calculated with allowance for orbital angular momentum loss due to a magnetic stellar wind and gravitational wave radiation. Stars with chemical compositions corresponding to disk and bulge objects are considered. The influence of induced stellar wind on the evolution of secondary components is investigated. The results of the calculations make it possible to explain the period distribution of cataclysmic variables and matter transfer rates observed in them and in low-mass X-ray sources.

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