Two-dimensional Parameter Relationships for W UMa-type Systems Revisited

Author:

Poro AtilaORCID,Paki EhsanORCID,Alizadehsabegh AilarORCID,Khodadadilori MehdiORCID,Salehian Selda RanjbarORCID,Hedayatjoo MahyaORCID,Hashemi FatemehORCID,Dashti YasamanORCID,Mohammadizadeh FatemehORCID

Abstract

Abstract Reviewing the empirical and theoretical parameter relationships between various parameters is a good way to understand more about contact binary systems. In this investigation, two-dimensional (2D) relationships for PM V(system), PL 1,2, M 1,2L 1,2, and qL ratio were revisited. The sample used is related to 118 contact binary systems with an orbital period shorter than 0.6 days whose absolute parameters were estimated based on the Gaia Data Release 3 parallax. We reviewed previous studies on 2D relationships and updated six parameter relationships. Therefore, Markov chain Monte Carlo and Machine Learning methods were used, and the outcomes were compared. We selected 22 contact binary systems from eight previous studies for comparison, which had light curve solutions using spectroscopic data. The results show that the systems are in good agreement with the results of this study.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Estimating the absolute parameters of W UMa-type binary stars using Gaia DR3 parallax;New Astronomy;2024-08

2. First Light Curve Analysis of NSVS 8294044, V1023 Her, and V1397 Her Contact Binary Systems;Research in Astronomy and Astrophysics;2024-05-01

3. BSN: Photometric Light Curve Analysis of Two Contact Binary Systems LS Del and V997 Cyg;Research in Astronomy and Astrophysics;2024-04-01

4. Global Parameters of Eight W UMa-type Binary Systems;Publications of the Astronomical Society of the Pacific;2024-02-01

5. Period–Luminosity Relationship for δ Scuti Stars Revisited;Research in Astronomy and Astrophysics;2024-01-31

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