Magnetic fields in O-, B- and A-type stars on the main sequence
arXiv:1411.7549 · doi:10.1051/epjconf/201510105001
Abstract
In this review, the latest observational results on magnetic fields in main-sequence stars with radiative envelopes are summarised together with the theoretical works aimed at explaining them.
CoRoT Symposium 3 / Kepler KASC-7 joint meeting, Toulouse, July 2014. To be published by EPJ Web of Conferences
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