Publication | Open Access
A solar-like magnetic cycle on the mature K-dwarf 61 Cygni A (HD 201091)
89
Citations
61
References
2016
Year
EngineeringSolar ConvectionSolar-like Magnetic CycleSolar PhysicDynamo GenerationMagnetohydrodynamicsSolar ActivityPhotometryPhysicsCool StarsCygni AMagnetarAstrophysicsSolar VariabilityNatural SciencesStellar StructureMature K-dwarf 61Magnetic CyclesAstrophysical Plasma
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.
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