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Cited article:

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Long-term Photometric Variability in Kepler Full-frame Images: Magnetic Cycles of Sun–like Stars

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The most plausible explanation of the cyclic period changes in close binaries: the case of the RS CVn-type binary WW Dra

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Monthly Notices of the Royal Astronomical Society no (2010)
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Long-term starspot evolution, activity cycle and orbital period variation of RT Lacertae

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Astronomy & Astrophysics 386 (2) 583 (2002)
https://doi.org/10.1051/0004-6361:20020301