Evolution of binaries with ultra-short periods - Systematic study

Details Evolution of binaries with ultra-short periods - Systematic study Evolution of binaries with ultra-short periods - Systematic study

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.151..125f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 151, no. 1, Jan. 1989, p. 125-134.

Astronomy and Astrophysics

Astrophysics

32

Roche Limit, Stellar Evolution, Stellar Mass, X Ray Binaries, Cataclysmic Variables, Gravitational Waves, Main Sequence Stars, Stellar Luminosity, Stellar Winds

Scientific paper

The evolution of low-mass binaries is studied for the case when the secondary fills its Roche lobe at the stage of core hydrogen exhaustion. The variation of the surface chemical composition of the secondary is studied and the values of the surface hydrogen content are shown as a function of the orbital period. It is proposed that MXB 1916-05 is the progenitor of the system MXB 1820-30 and is ascending toward short orbital periods.

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