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• W4300503552 abstract "Context. HD 208472 is among the most active RS CVn binaries with cool starspots. Decade-long photometry has shown that the spots seem to change their longitudinal appearance with a period of about six years, coherent with brightness variations." @default.
• W4300503552 created "2022-10-03" @default.
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• W4300503552 date "2016-09-01" @default.
• W4300503552 modified "2023-10-15" @default.
• W4300503552 title "Time-series Doppler imaging of the red giant HD 208472" @default.
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• W4300503552 doi "https://doi.org/10.1051/0004-6361/201628545" @default.
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