WZ Cygni: a Marginal Contact Binary in a Triple System?
Jae Woo Lee, Seung-Lee Kim, Chung-Uk Lee, Ho-Il Kim, Jang-Ho Park, and, Tobias Cornelius Hinse

TL;DR
This study presents new multiband photometry and period analysis of WZ Cyg, revealing it as a marginal contact binary in a triple system with ongoing mass transfer and a tertiary companion, contributing to understanding of binary evolution.
Contribution
It provides detailed photometric and period analysis of WZ Cyg, identifying its marginal contact status and the presence of a tertiary companion, which are novel insights into its evolutionary stage.
Findings
WZ Cyg is a marginal contact binary with poor thermal contact.
The orbital period shows a continuous increase and a sinusoidal variation.
A low-mass tertiary companion likely causes the observed light-travel-time effect.
Abstract
We present new multiband CCD photometry for WZ Cyg made on 22 nights in two observing seasons of 2007 and 2008. Our light-curve synthesis indicates that the system is in poor thermal contact with a fill-out factor of 4.8% and a temperature difference of 1447 K. Including our 40 timing measurements, a total of 371 times of minimum light spanning more than 112 yr were used for a period study. Detailed analysis of the -- diagram showed that the orbital period has varied by a combination with an upward parabola and a sinusoid. The upward parabola means the continuous period increase and indicates that some stellar masses are thermally transferred from the less to the more massive primary star at a rate of about 5.80 M yr. The sinusoidal variation with a period of 47.9 yr and a semi-amplitude of 0.008 d can be interpreted most likely as the…
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