Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani
T.S. Metcalfe, A.P. Buccino, B.P. Brown, S. Mathur, D.R. Soderblom,, T.J. Henry, P.J.D. Mauas, R. Petrucci, J.C. Hall, S. Basu

TL;DR
This study confirms a 3-year magnetic activity cycle in epsilon Eridani, analyzes 45 years of data revealing coexisting cycles, and discusses implications for stellar dynamo theories and the Sun's unique magnetic behavior.
Contribution
It provides the first detailed long-term analysis of epsilon Eridani's magnetic cycles, suggesting multiple dynamo mechanisms and revising understanding of stellar magnetic activity.
Findings
Confirmation of a 3-year cycle in epsilon Eri.
Detection of coexisting 3-year and 13-year cycles.
Implication that the Sun's rotational history influences its magnetic peculiarities.
Abstract
The active K2 dwarf epsilon Eri has been extensively characterized, both as a young solar analog and more recently as an exoplanet host star. As one of the nearest and brightest stars in the sky, it provides an unparalleled opportunity to constrain stellar dynamo theory beyond the Sun. We confirm and document the 3 year magnetic activity cycle in epsilon Eri originally reported by Hatzes and coworkers, and we examine the archival data from previous observations spanning 45 years. The data show coexisting 3 year and 13 year periods leading into a broad activity minimum that resembles a Maunder minimum-like state, followed by the resurgence of a coherent 3 year cycle. The nearly continuous activity record suggests the simultaneous operation of two stellar dynamos with cycle periods of 2.95+/-0.03 years and 12.7+/-0.3 years, which by analogy with the solar case suggests a revised…
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