BVR observations and period variation of the near-contact binary ZZ Aurigae |
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Authors: | Kyu-Dong Oh Chun-Hwey Kim Woo-Baik Lee Ho-il Kim Young Woon Kang |
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Affiliation: | Department of Earth Sciences, Chonnam National University, Kwangju 500-757, Korea;Department of Astronomy and Space Sciences, College of Natural Science and Institute for Basic Science Research, Chungbuk National University, Cheongju, 361-763, Korea;Korea Astronomy Observatory, Taejon 305-348, Korea;Department of Astronomy, Sejong University, Seoul 143-747, Korea |
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Abstract: | BVR light curves of ZZ Aurigae were obtained with the 60-cm Cassegrain reflector at the Sobaek Observatory, Korea, between 2000 February and 2001 February. All collected times of minimum light, including our observations, were used for the period study. The period variation could be of quasi-sinusoidal form superposed on an upward parabola. A continuous period increase of d P /d t =+2.3 × 10−8 d yr−1 was determined for ZZ Aur. The period of quasi-sinusoidal variation is about ∼26–31 yr. Photometric solutions were found using the Wilson–Devinney method. The Roche configuration of ZZ Aur is that of an Algol-type semidetached system where the primary star nearly fills its Roche lobe and the secondary star fills its lobe. The spot model was used to explain the asymmetry in the light curve known as the O'Connell effect. |
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Keywords: | binaries: eclipsing stars: chromospheres stars: individual: ZZ Aurigae stars: spots |
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