Abstract
The photometric variability RU Peg was studied based on 15 498 visual observations from the AFOEV and VSOLJ databases since 1934 (JD 2427762-51202). The long-term cycles in the cycle duration and brightness of the low state may be interpreted either as the solar-type activity cycles of the secondary or by the presence of third body.
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Chinarova, L.L., Andronov, I.L. (2003). Variations of the Outburst Characteristics of the Dwarf Nova Ru Peg. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_100
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DOI: https://doi.org/10.1007/978-94-010-0215-8_100
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