Evolution of low mass close binaries with orbital momentum losses

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

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236....7t&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 7-16 (SEE N86-20287 10-93)

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Angular Momentum, Cataclysmic Variables, Stellar Evolution, Stellar Mass Ejection, Gravitational Waves, Stellar Winds, X Ray Sources

Scientific paper

The formation and evolution of low-mass (M2 M1 or = 1.5 solar mass) close binaries influenced by angular momentum loss by radiation of gravitational waves and magnetic stellar wind is reviewed. The frequency of formation of cataclysmic variables and low-mass X-ray sources is 0.005 and 0.00000003 per year, respectively. Results of evolutionary computations of secondaries are presented, which explain the existence of 2 to 3h orbital period gap, 80m minimal period, as well as the existence of unique ultrashort period systems with 15m or = P or = 1h.

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