The contact binary VW Cephei revisited: surface activity and period variation
T. Mitnyan (1), A. B\'odi (1, 2), T. Szalai (1), J. Vink\'o (1 and, 2), K. Szatm\'ary (1), T. Borkovits (2, 3), B. I. B\'ir\'o (3), T., Heged\"us (3), K. Vida (2), A. P\'al (2) ((1) University of Szeged, (2), Konkoly Observatory

TL;DR
This study provides new spectroscopic and photometric data on VW Cephei, revises its physical parameters, and explores mechanisms like magnetic activity and mass transfer to explain its period variations and surface activity.
Contribution
It offers a comprehensive re-analysis of VW Cephei using new data, proposing a flip-flop activity phenomenon and evaluating different models for period changes.
Findings
Primary component shows higher activity and spottedness.
Flip-flop phenomenon may explain activity variations.
Mass transfer likely causes period variation.
Abstract
Context. Despite the fact that VW Cephei is one of the well-studied contact binaries in the literature, there is no fully consistent model available that can explain every observed property of this system. Aims. Our motivation is to obtain new spectra along with photometric measurements, to analyze what kind of changes may have happened in the system in the past two decades, and to propose new ideas for explaining them. Methods. For the period analysis we determined 10 new times of minima from our light curves, and constructed a new OC diagram of the system. Radial velocities of the components were determined using the cross-correlation technique. The light curves and radial velocities were modelled simultaneously with the PHOEBE code. All observed spectra were compared to synthetic spectra and equivalent widths of the H line were measured on their differences. Results.…
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