Orbital Element Analysis of a Short Period Eclipsing Binary UV PISCIUM

Details Orbital Element Analysis of a Short Period Eclipsing Binary UV PISCIUM Orbital Element Analysis of a Short Period Eclipsing Binary UV PISCIUM

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jass...13...72h&link_type=abstract

Journal of Astronomy and Space Science, vol. 13, no. 1, p.72-78.

Astronomy and Astrophysics

Astronomy

Scientific paper

We evaluated the orbital elements of BV light curves of a short period RS CVn type eclipsing binary system UV Picsium that shows complicated light variation, by analyzing with the Winson-Devinney's differential correction method. Because the analyzed light curves shown large light variation at outside eclipse region, we assumed spotted region of the primary component and calculated its position and size. The results show the UV Psc is a detached binary system of nearly the same radii and the primary component has high mass with high temperature. However this result is not consistant with customary stellar models, thus requires more observational data to confirm this problem.

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