An application of a solar-type dynamo model for Epsilon Eridani
A. P. Buccino,
L. Sraibman,
P. Olivar
et al.
Abstract:During the last decade, the relation between activity cycle periods with stellar parameters has received special attention. The construction of reliable registries of activity reveals that solar type stars exhibit activity cycles with periods from few years to decades and, in same cases, long and short activity cycles coexist suggesting that two dynamos could operate in these stars. In particular, ε Eridani is an active young K2V star (0.8 Gyr), which exhibits a short and long-term chromospheric cycles of ∼3 a… Show more
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