Analysis of the eclipsing binary ST Carinae using the SIMPLEX algorithm

Astronomy and Astrophysics – Astronomy

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Eclipsing Binary Stars, Light Curve, Algorithms, Astronomical Models, Kepler Laws, Orbital Elements

Scientific paper

This work presents the analyses of two UBV data sets for the Algol binary ST Carinae, presenting a homogeneous study of all the data. The light-curve parameters for the system are derived using the Wilson-Devinney model (1917), with the SIMPLEX algorithm as an optimization procedure, and a mass ratio of q=0.54 is obtained. The primary has colors consistent with a B9.5 V primary, and the solution indicates that the secondary is an F subgiant (Te=6200 K) that fills its Roche lobe. The application of Kepler's law (using the observed period and the mass ratio determined in this investigation) indicates that the absolute dimensions for the components are normal for their respective classes. A description of SIMPLEX is given, and its advantages for the solution of eclipsing binary parameters are discussed.

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