Krzeminsky's optical candidate for CEN X-3

Details Krzeminsky's optical candidate for CEN X-3 Krzeminsky's optical candidate for CEN X-3

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pasau...2..289w&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 8th, Hobart, Australia, May 22-24, 1974.) Astronomical Society of Au

Astronomy and Astrophysics

Astronomy

Eclipsing Binary Stars, Light Sources, Roche Limit, Stellar Radiation, X Ray Stars, Ellipsoids, Light Curve, Optical Properties, Orbital Elements, Pulsars, Stellar Mass Ejection, X Ray Sources

Scientific paper

A Roche lobe analysis was conducted in order to determine whether the available observational data concerning the star considered by Krzeminsky (1973) are consistent with the various constraints imposed by the X-ray data. The light curve synthesis program described by Strittmatter et al. (1973) was used in the analysis. It was found that the primary must be in near contact with its inner critical Roche lobe.

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