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Cited article:

TESS photometry, radial velocity, and orbital period investigations of four eclipsing contact binaries

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

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OO Leo: An Active Contact Binary with Possible Solar-like Differential Rotation

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The Astrophysical Journal 971 (1) 113 (2024)
https://doi.org/10.3847/1538-4357/ad571e

An Investigation of six contact binary systems and a semi-detached one

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https://doi.org/10.1016/j.newast.2024.102228

First photometric and orbital period investigations of four W UMa-type eclipse binaries

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Publications of the Astronomical Society of Australia 39 (2022)
https://doi.org/10.1017/pasa.2022.53

Case AD, AR, and AS binary evolution and their possible connections with W UMa binaries

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Monthly Notices of the Royal Astronomical Society 492 (2) 2731 (2020)
https://doi.org/10.1093/mnras/stz3578

The detached-binary channel for the formation of contact binaries

Dengkai Jiang, Zhanwen Han and Lifang Li
Monthly Notices of the Royal Astronomical Society 438 (1) 859 (2014)
https://doi.org/10.1093/mnras/stt2252

On the origin of W UMa type contact binaries – a new method for computation of initial masses

M. Yildiz and T. Doğan
Monthly Notices of the Royal Astronomical Society 430 (3) 2029 (2013)
https://doi.org/10.1093/mnras/stt028

THE ANTICORRELATED NATURE OF THE PRIMARY AND SECONDARY ECLIPSE TIMING VARIATIONS FOR THEKEPLERCONTACT BINARIES

K. Tran, A. Levine, S. Rappaport, et al.
The Astrophysical Journal 774 (1) 81 (2013)
https://doi.org/10.1088/0004-637X/774/1/81

Energy transfer and its effects on the secondaries in W Ursae Majoris type contact binaries

Dengkai Jiang, Zhanwen Han, Tianyu Jiang and Lifang Li
Monthly Notices of the Royal Astronomical Society 396 (4) 2176 (2009)
https://doi.org/10.1111/j.1365-2966.2009.14852.x

Structure and evolution of W UMa-type systems

Lifang Li, Fenghui Zhang, Zhanwen Han, Dengkai Jiang, and Tianyu Jiang
Proceedings of the International Astronomical Union 4 (s252) 423 (2008)
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Structure and evolution of low-mass W Ursae Majoris type systems - III. The effects of the spins of the stars

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ABSOLUTE PARAMETERS AND MASS-RADIUS-LUMINOSITY RELATIONS FOR THE SUB-TYPES OF W UMα BINARIES

N. S. AWADALLA and M. A. HANNA
Journal of The Korean Astronomical Society 38 (2) 43 (2005)
https://doi.org/10.5303/JKAS.2005.38.2.043

Structure and evolution of low-mass W Ursae Majoris type systems - II. With angular momentum loss

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Monthly Notices of the Royal Astronomical Society 355 (4) 1383 (2004)
https://doi.org/10.1111/j.1365-2966.2004.08457.x