Photometric study of three ultrashort-period contact binaries
L. Liu, S.-B., E. Fernandez Lajus, A. Essam, M. A. El-Sadek, and X., Xiong

TL;DR
This study presents high-precision photometric observations and modeling of three ultrashort-period contact binaries, revealing their evolutionary states and the presence of cool spots, with a comparative analysis of 28 similar systems.
Contribution
It provides detailed photometric analysis and modeling of three USPCBs, including their fill-out factors and spot activity, and compares them with a larger sample to understand their evolutionary stages.
Findings
Most USPCBs are in shallow contact with f<20%.
Deep contact USPCBs are rare and possibly merging.
One system is a zero contact binary in thermal equilibrium.
Abstract
We carried out high-precision photometric observations of three eclipsing ultrashortperiod contact binaries (USPCBs). Theoretical models were fitted to the light-curves by means of the Wilson-Devinney code. The solutions suggest that the three targets have evolved to a contact phase. The photometric results are as follows: a) 1SWASP J030749.87-365201.7, q=0.439\pm0.003, f=0.0\pm3.6%; b) 1SWASP J213252.93-441822.6, q=0.560\pm0.003, f=14.2\pm1.9%; c) 1SWASP J200059.78+054408.9, q=0.436\pm0.008, f=58.4\pm1.8%. The light curves show O'Connell effects, which can be modeled by assumed cool spots. The cool spots models are strongly supported by the night-to-night variations in the I-band light curves of 1SWASP J030749.87-365201.7. For a comparative study, we collected the whole set of 28 well-studied USPCBs with P < 0.24 day. Thus, we found that most of them (17 of 28) are in shallow contact…
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