201. The first photometric investigation of the contact binary OQ Cam
- Author
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Kai Li, Qi-Qi Xia, Xing Gao, Yuan Liu, Lin-Qiao Jiang, and Ya-Ni Guo
- Subjects
Physics ,Oscillation theory ,Degree (graph theory) ,010308 nuclear & particles physics ,Star (game theory) ,FOS: Physical sciences ,Potential candidate ,Astronomy and Astrophysics ,Contact binary ,Astrophysics ,Light curve ,Orbital period ,01 natural sciences ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,0103 physical sciences ,Thermal relaxation ,010303 astronomy & astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
The first charge-coupled device photometric light curves in B, V, R${_c}$, and I${_c}$ bands of the short-period contact binary star OQ Cam are presented. Through analyzing the light curves with the Wilson-Devinney code, it is found that OQ Cam is a W-type shallow contact binary star with a contact degree of f =20.2%. Based on the O-C analyzing, the orbit period displays a long term increasing with a rate of $dP/dt=4.40\times10{^{-7}} day \cdot year{^{-1}}$. The increasing in orbit period can be interpreted by mass transfer from the less massive component to the more massive one. As the orbit period increasing, OQ Cam would evolve from the present shallow contact configuration to a none contact stage. So it may be a potential candidate to confirm the thermal relaxation oscillation theory., 11 pages, 6 figures, and 5 tables, accepted by RAA
- Published
- 2020
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