Photometric investigation of near-contact binary FR Ori

Details Photometric investigation of near-contact binary FR Ori Photometric investigation of near-contact binary FR Ori

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..240r.126g&link_type=abstract

Binary Stars as Critical Tools and Tests in Contemporary Astrophysics, International Astronomical Union. Symposium no. 240, he

Astronomy and Astrophysics

Astrophysics

Scientific paper

Analysis of UBV photoelectric photometry for the eclipsing binary FR Ori using new observational data is presented. The light changes are not caused only due to existence of the eclipses, but also due to activity in the system. The U, B and V light curves were analysed by the Wilson-Devinney codes to derive the geometrical and physical parameters of the system.

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