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Cited article:

Magnetic activities on two single-lined RS Canum Venaticorum binaries IM Pegasi and σ Geminorum

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A Method to Search for Black Hole Candidates with Giant Companions by LAMOST

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The Astrophysical Journal Letters 872 (2) L20 (2019)
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General Model for Light Curves of Chromospherically Active Binary Stars∗

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Time‐series analysis of long‐term photometry of BM Canum Venaticorum

L. Siltala, L. Jetsu, T. Hackman, G. W. Henry, L. Immonen, P. Kajatkari, J. Lankinen, J. Lehtinen, S. Monira, S. Nikbakhsh, A. Viitanen, J. Viuho and T. Willamo
Astronomische Nachrichten 338 (4) 453 (2017)
https://doi.org/10.1002/asna.201613205

DETECTING THE COMPANIONS AND ELLIPSOIDAL VARIATIONS OF RS CVn PRIMARIES. I.σGEMINORUM

Rachael M. Roettenbacher, John D. Monnier, Gregory W. Henry, et al.
The Astrophysical Journal 807 (1) 23 (2015)
https://doi.org/10.1088/0004-637X/807/1/23

Initial Results from the USNO Dispersed Fourier Transform Spectrograph

Arsen R. Hajian, Bradford B. Behr, Andrew T. Cenko, et al.
The Astrophysical Journal 661 (1) 616 (2007)
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A Large Millimeter Flare on the RS CVn Binary σ Geminorum

Joanna M. Brown and Alexander Brown
The Astrophysical Journal 638 (1) L37 (2006)
https://doi.org/10.1086/500929

Quiescent and Flaring Structure in RS Canum Venaticorum Stars

J. Sanz‐Forcada, N. S. Brickhouse and A. K. Dupree
The Astrophysical Journal 570 (2) 799 (2002)
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An Optical Region Elemental Abundance Analysis of the HgMn Type Star HR 7775

Glenn M. Wahlgren, Linus Dolk, Gabriele Kalus, et al.
The Astrophysical Journal 539 (2) 908 (2000)
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