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2017MNRAS.471L..96J - Mon. Not. R. Astron. Soc., 471, L96-L100 (2017/October-2)
The relation between stellar magnetic field geometry and chromospheric activity cycles - I. The highly variable field of ε Eridani at activity minimum.
JEFFERS S.V., BORO SAIKIA S., BARNES J.R., PETIT P., MARSDEN S.C., JARDINE M.M. and VIDOTTO A.A.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): techniques: polarimetric - stars: activity - stars: individual: ε Eridani - stars: magnetic field - stars: solar-type - stars: solar-type
Simbad objects: 2
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