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- W2117074785 abstract "We present the long-term multi-colour photometry of MM Her which is one of the first members of the RS CVn-type of eclipsing binary systems. We took advantage of its photometry-spanning 33 years to evaluate its long-term variation, which is caused by the evolution of the activity structures located on the surface of the cooler component. In this study we found that the long-term variation in the brightness, colour, and amplitude of seasonal light curves over the years could be represented by two periods: one of which is of around 22.5 years, and is similar to all in this regard, but the other is a period value of about 9.5 years for the brightness variation, and of about 7.5 years for the variation in colour and amplitude. The analysis of the spot minimum phases gives a migration period of approximately 7.8 years. We also presented a new light curve analysis solution, and improved its light elements in this study. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
- W2117074785 created "2016-06-24" @default.
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- W2117074785 date "2013-03-01" @default.
- W2117074785 modified "2023-10-17" @default.
- W2117074785 title "One of the first members of RS CVn-type systems: MM Herculis" @default.
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- W2117074785 doi "https://doi.org/10.1002/asna.201211737" @default.
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