The relation between stellar magnetic field geometry and chromospheric activity cycles - I. The highly variable field of e Eridani at activity minimum (2017)

First Author: Jeffers S
Attributed to:  Astronomy and Planetary Sciences at the Open University (APSOU) funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnrasl/slx097

Publication URI: http://dx.doi.org/10.1093/mnrasl/slx097

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society: Letters

Issue: 1