EPJ Web of Conferences
Volume 101, 2015The Space Photometry Revolution – CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
|Number of page(s)||5|
|Section||Session 5 - Stellar activity and rotation|
|Published online||23 September 2015|
Magnetic fields in O-, B- and A-type stars on the main sequence
1 Institut d’Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 17, Bât B5c, 4000, Liège, Belgium
2 LESIA, Observatoire de Paris, CNRS UMR 8109, UPMC, Univ. Paris Diderot, 5 place Jules Janssen, 92195, Meudon Cedex, France
a e-mail: email@example.com
b F.R.S.-FNRS Postdoctoral Researcher, Belgium
Published online: 23 September 2015
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.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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