Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-12-21
Astronomy and Astrophysics
Astrophysics
6 pages, 2 figures. Proceedings of Solar Polarisation Workshop #5
Scientific paper
A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magnetic fields. The large majority of such stars, however, show no evidence for magnetic fields, even when observed with very high precision. In this paper we describe a simple model, motivated by qualitatively new observational results, that provides a natural physical explanation for the small fraction of observed magnetic stars.
Auriere Michel
Bagnulo Stefano
Bale K.
Bon Hoa Hui A.
Dintrans Boris
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