A new light synthesis optimization program - Test on simulated Algol data

Details A new light synthesis optimization program - Test on simulated Algol data A new light synthesis optimization program - Test on simulated Algol data

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ssrv...50..269l&link_type=abstract

(IAU, NSERC, Canadian Institute of Theoretical Astrophysics, et al., Colloquium on Algols, 107th, Sidney, Canada, Aug. 15-19, 19

Astronomy and Astrophysics

Astrophysics

1

Eclipsing Binary Stars, Light Curve, Optimization, Simulation, Automation, Iterative Solution

Scientific paper

Simulation of light curve effects in Algol systems that are near contact or that may evolve into contact requires a different model than the tri-axial ellipsoid used in many current studies. A new light synthesis optimization program, based on the Roche model, satisfies the model requirements and determines system parameters with excellent accuracy, given a sufficiently large set of observations. A widely used criterion for stopping iterative solutions is inadequate. A working criterion is proposed as a replacement.

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