Computer Analysis and Modeling of an Eclipsing Binary Star

Details Computer Analysis and Modeling of an Eclipsing Binary Star Computer Analysis and Modeling of an Eclipsing Binary Star

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..tsf..bc12m&link_type=abstract

American Physical Society, Texas Section Fall Meeting, October 10-11, 1997, abstract #BC.12

Physics

Scientific paper

Between September 1995 and July 1996, a detailed light curve of the Beta
Lyra-type eclipsing binary star 68 Herculis was made by the authors.
This data is analyzed to determine a period and epoch for the star,
search for evolutionary changes in the system, and physically model the
orbiting pair of stars.

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