Periods of activity cycles in late-type stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrophysics, Cycles, Dynamo Theory, Late Stars, Stellar Rotation, Angular Velocity, Convection, Dynamic Characteristics, Stellar Envelopes, Stellar Magnetic Fields

Scientific paper

The mean magnetic field dynamo theory is utilized to obtain the
qualitative dependence of the period of activity on the angular velocity
of rotation for stars with sufficiently extensive convective shells. The
dependence of the cycle period on the spectral class is also discussed.

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