Evolution of low-mass close binaries - The mininum orbital period

Details Evolution of low-mass close binaries - The mininum orbital period Evolution of low-mass close binaries - The mininum orbital period

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..123t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Feb. 1985, p. 123-132) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Jan.-Feb

Astronomy and Astrophysics

Astronomy

15

Binary Stars, Stellar Evolution, Stellar Mass, Stellar Orbits, Angular Momentum, Cataclysmic Variables, Gravitational Waves, Mass Transfer, X Ray Binaries

Scientific paper

The evolution of low-mass close binaries with compact primaries and slightly evolved secondaries has been studied numerically taking into account the angular momentum loss due to a magnetic stellar wind and radiation of gravitational waves. The evolution of such systems leads to the formation of close binaries with orbital periods ≡20m - 80m, the mass exchange rate up to ≡10-9M_sun;/yr, and to the formation of a low-mass helium dwarf. Thus ultrashort-period cataclysmic and X-ray systems with periods lower than ≡80m can be formed.

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