Orbital Period Variation Analysis of the HS 0705+6700 Post-Common Envelope Binary
Huseyin Er, Aykut \"Ozd\"onmez, Ilham Nasiroglu, Muhammet Emir Kenger

TL;DR
This study analyzes 24 years of eclipse timing data for the binary system HS 0705+6700, exploring orbital period variations and potential additional bodies, with findings suggesting complex dynamics and the need for further observations.
Contribution
It provides the longest observational baseline for HS 0705+6700 and models the orbital variations considering multiple hypotheses, including multiple brown dwarfs and the Applegate mechanism.
Findings
Significant deviations in the O-C diagram over 24 years.
Models with multiple brown dwarfs fit the data statistically.
The Applegate mechanism alone cannot explain the period variations.
Abstract
To detect additional bodies in binary systems, we performed a potent approach of orbital period variation analysis. In this work, we present 90 new mid-eclipse times of a short-period eclipsing binary system. Observations were made using two telescopes from 2014 to 2024, extending the time span of the O-C diagram to 24 years. The data obtained in the last seven years indicate significant deviations in the O-C diagram from the models obtained in previous studies. We investigated whether this variation could be explained by mechanisms such as the LTT effect or Applegate. To investigate the cyclic behaviour observed in the system with the LTT effect, we modelled the updated O-C diagram using different models including linear/quadratic terms and additional bodies. The updated O-C diagram is statistically consistent with the most plausible solutions of models that include multiple brown…
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