Discovery of two rotational modulation periods from a young hierarchical triple system

GW~Ori is a young hierarchical triple system located in \(\lambda\) Orionis, consisting of a binary (GW~Ori\,A and B), a tertiary star (GW~Ori\,C) and a rare circumtriple disk. Due to the limited data with poor accuracy, several short-period signals were detected in this system, but the values from...

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Bibliographic Details
Published in:arXiv.org 2023-05
Main Authors: Yu-Tao, Chen, Hai-Jun Tian, Fang, Min, Xiao-Xiong, Zuo, Bird, Sarah A, Liu, Di, Xin-Yu, Zhu, Zhang, Peng, Gao-Chao, Liu, Cui, Sheng
Format: Article
Language:English
Subjects:
Binary stars
Deposition
Extrasolar planets
Light curve
Modulation
Planet detection
Transit
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Summary:GW~Ori is a young hierarchical triple system located in \(\lambda\) Orionis, consisting of a binary (GW~Ori\,A and B), a tertiary star (GW~Ori\,C) and a rare circumtriple disk. Due to the limited data with poor accuracy, several short-period signals were detected in this system, but the values from different studies are not fully consistent. As one of the most successful transiting surveys, the Transiting Exoplanet Survey Satellite (TESS) provides an unprecedented opportunity to make a comprehensive periodic analysis of GW~Ori. In this work we discover two significant modulation signals by analyzing the light curves of GW~Ori's four observations from TESS, i.e., 3.02 \(\pm\) 0.15\,d and 1.92 \(\pm\) 0.06\,d, which are very likely to be the rotational periods caused by starspot modulation on the primary and secondary components, respectively. We calculate the inclinations of GW~Ori\,A and B according to the two rotational periods. The results suggest that the rotational plane of GW~Ori\,A and B and the orbital plane of the binary are almost coplanar. We also discuss the aperiodic features in the light curves; these may be related to unstable accretion. The light curves of GW~Ori also include a third (possible) modulation signal with a period of 2.51\(\pm\)0.09\,d, but the third is neither quite stable nor statistically significant.
ISSN:2331-8422