The Parameters of the X-Ray Binary System HD253919 = 4U1700-37

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

A self-consistent model of the X-ray binary HD 153919 = 4U 1700-37 for the interpretation of the optical light curve corrected for the eclipse effects is developed. In the framework of this model reliable values of the parameters for this system are determined. The eclipses of the optical star by the accretion disk are taken into account, allowing to describe the observed amplitude and the difference between the minima of the observed optical light curve of HD 153919.

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