The Synthesis of Close-Binary Light Curves IV. An Application to TX Ursae Majoris and MR Cygni

Details The Synthesis of Close-Binary Light Curves IV. An Application to TX Ursae Majoris and MR Cygni The Synthesis of Close-Binary Light Curves IV. An Application to TX Ursae Majoris and MR Cygni

Jan 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..20..123h&link_type=abstract

Astrophysics and Space Science, Volume 20, Issue 1, pp.123-148

Astronomy and Astrophysics

Astrophysics

26

Scientific paper

A full description is given of the theory used in light curve synthesis, for binary stars showing various degrees of interaction. For strongly interacting pairs, an iterative mutual heating calculation is introduced. Detailed models are derived by these methods, and discussed, for the weakly interacting system TX U Ma and the strongly interacting system MR Cyg. A critical appraisal is given of this method of light curve synthesis and its results.

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