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• W2411330540 abstract "Context. The long-term monitoring of magnetic cycles in cool stars is a key diagnostic in understanding how dynamo generation and amplification of magnetic fields occur in stars similar in structure to the Sun." @default.
• W2411330540 created "2016-06-24" @default.
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• W2411330540 date "2016-10-01" @default.
• W2411330540 modified "2023-10-14" @default.
• W2411330540 title "A solar-like magnetic cycle on the mature K-dwarf 61 Cygni A (HD 201091)" @default.
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• W2411330540 doi "https://doi.org/10.1051/0004-6361/201628262" @default.
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