New results of numerical simulations of X ray binaries evolution

Details New results of numerical simulations of X ray binaries evolution New results of numerical simulations of X ray binaries evolution

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..653t&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 653-656 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Computerized Simulation, Neutron Stars, Stellar Evolution, Stellar Luminosity, X Ray Binaries, Active Galaxies, Stellar Mass Accretion, Stellar Models, X Ray Astronomy

Scientific paper

The results of numerical calculations of the evolution of Neutron Star (NS) in close binaries are presented. The detailed analysis of the NS evolution uses accurate evolutionary tracks for optical companion. By using less accurate evolutionary tracks for normal stars the simulation of the joint evolution of 100,000 binaries is performed. The evolution of total X ray luminosity caused by accreting neutron stars was calculated for different types of galaxies.

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