An analysis of the optical light curve of the X-ray binary 3U 1653+35

Details An analysis of the optical light curve of the X-ray binary 3U 1653+35 An analysis of the optical light curve of the X-ray binary 3U 1653+35

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.151..181a&link_type=abstract

Astrophysics and Space Science, Volume 151, Issue 2, pp.181-207

Astronomy and Astrophysics

Astrophysics

Scientific paper

The purpose of this paper is to provide an estimate of several parameters of X-ray binary system 3U 1653+35, based a study of the optical light curve of the companion of HZ Her. The introductory section gives a general outline of the problem and deals with the general method of estimation of the parameters. In Section 2, the reflection effect in close binary systems is demonstrated in the end of this section we first introduce a new method of evaluation of reflection effect in close binary systems. Section 3 gives an analysis of the optical curve of the X-ray binary system 3U 1653+35, and general discussion.

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