The relation between stellar magnetic field geometry and chromospheric activity cycles – I. The highly variable field of ε Eridani at activity minimum
2017 | journal article. A publication with affiliation to the University of Göttingen.
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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. & Vidotto, A. A. (2017)
Monthly notices of the Royal Astronomical Society. Letters, 471(1) pp. L96-L100. DOI: https://doi.org/10.1093/mnrasl/slx097
