Photometric study and period analysis of the contact binary XZ Leonis
Changqing Luo, Xiaobin.Zhang, Licai Deng, Kun Wang, Yangping Luo

TL;DR
This study presents detailed photometric and period analysis of the contact binary XZ Leo, revealing its physical parameters, orbital period increase, and evolutionary status, supporting the Thermal Relaxation Oscillation theory.
Contribution
It provides a comprehensive photometric and orbital analysis of XZ Leo, including new light curves, revised system parameters, and long-term period behavior, which was not previously studied in detail.
Findings
XZ Leo is an A-type contact binary with 24% contact degree.
The orbital period is increasing at a rate of 6.12×10^{-8} days/year.
The system is likely to evolve into a broken-contact stage in 1.56 million years.
Abstract
We present multi-color CCD photometry of the neglected contact binary XZ Leo. Completely covered VRI band light curves and four times of minimum light were obtained. Combining the photometric and previously published radial velocity data, a revised photometric analysis was carried out for the binary system by applying the Wilson-Devinney code. With a hot spot placed on the massive primary component near the neck region of the common envelope, the light curves were satisfactorily modeled. The photometric solution combined with the radial velocity solution reveals that XZ Leo is an A-type contact binary with a degree of contact of 24(. The absolute parameters of the components were determined as M_1 = 1.74(0.06)M_\odot, M_2 = 0.61(0.02)M_\odot, R_1 = 1.69(0.01)R_\odot, R_2 = 1.07()R_\odot, L_1 = 6.73() L_\odot, L_2 = 2.40(0.04)L_\odot. Based…
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