New Developments in Eclipsing Binary Light Curve Modeling

Details New Developments in Eclipsing Binary Light Curve Modeling New Developments in Eclipsing Binary Light Curve Modeling

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....5..163m&link_type=abstract

Experimental Astronomy, Volume 5, Issue 1-2, pp. 163-169

Astronomy and Astrophysics

Astronomy

Scientific paper

The light curve modeling of binary stars has continued to evolve since its founding by Henry Norris Russell (see Russell and Merrill 1952 and citations therein) nearly a century ago, accelerated in the 1950s by Kopal's introduction of Roche geometry into models and by the development of synthetic light curve computer code in the 1970's. Improved physics and the use of more kinds of observational input are providing another round of important advances that promise to enlarge our knowledge of both binary stars and ensembles containing them. Here we discuss the newer horizons of light curve modeling and the steps being taken toward them.

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