New Elements for Three Eclipsing X-Ray Binary Systems: HZ Herculis, Centaurus X-3, and VELA X-1

Details New Elements for Three Eclipsing X-Ray Binary Systems: HZ Herculis, Centaurus X-3, and VELA X-1 New Elements for Three Eclipsing X-Ray Binary Systems: HZ Herculis, Centaurus X-3, and VELA X-1

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..335a&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 3, p. 335-345 (1999).

Astronomy and Astrophysics

Astrophysics

Scientific paper

A contribution to the theoretical analysis of eclipsing x-ray binary systems and the calculation of physical and geometrical elements, are represented. The principle of this work is to make fitting between the observational light curve and the synthetic light curve built up in accordance with the Roche model, and to consider the elements of the best fitting as new elements. This method were applied to three systems, there are:

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