Abstract
BY Dra (MOVe+MOVe) and II Peg (K2IV-III) are well known non-eclipsing spectroscopic binary systems showing the low-amplitude quasi-periodic photometric variability that is typical of spotted stars.
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Rodonò, M., Pazzani, V., Cutispoto, G. (1983). Synopsis of by Dra and II Peg Light Curves: Variability and Possible Evidence of Differential Rotation. In: Byrne, P.B., Rodonò, M. (eds) Activity in Red-Dwarf Stars. Astrophysics and Space Science Library, vol 102. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7157-8_19
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DOI: https://doi.org/10.1007/978-94-009-7157-8_19
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