Duration of eclipses of a point source in X-ray binary systems with eccentric orbits

Details Duration of eclipses of a point source in X-ray binary systems with eccentric orbits Duration of eclipses of a point source in X-ray binary systems with eccentric orbits

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..356k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 356-364) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 2

Statistics

Computation

6

Computational Astrophysics, Eccentric Orbits, Eclipsing Binary Stars, Point Sources, X Ray Binaries, Algorithms, Astronomical Catalogs

Scientific paper

An algorithm for calculating the duration of the eclipse of a compact X-ray source in a close binary system with an eccentric orbit is presented, as well as tables of the dependence of the eclipse angle on the angle of inclination of the orbit for systems with different mass ratios of the components and for several values of the eccentricity of the orbit and its orientation in space. The influence of asynchronism of the rotation of the visible star on the eclipse duration is investigated.

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