Reference : Magnetic fields in beta Cep, SPB, and Be stars
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/156877
Magnetic fields in beta Cep, SPB, and Be stars
English
Schoeller, M. [> >]
Hubrig, S. [> >]
Briquet, Maryline [Université de Liège - ULiège > > >]
Ilyin, I. [> >]
1-Sep-2013
Proceedings of the Conference: "Putting A Stars into Context: Evolution, Environment, and Related Stars"
5497
No
International
"Putting A Stars into Context: Evolution, Environment, and Related Stars"
from 03-06-2013 to 07-06-2013
[en] Astrophysics - Solar and Stellar Astrophysics
[en] Recent observational and theoretical results emphasize the potential significance of magnetic fields for structure, evolution, and environment of massive stars. Depending on their spectral and photometric behavior, the upper main-sequence B-type stars are assigned to different groups, such as beta Cep stars and slowly pulsating B (SPB) stars, He-rich and He-deficient Bp stars, Be stars, BpSi stars, HgMn stars, or normal B-type stars. All these groups are characterized by different magnetic field geometry and strength, from fields below the detection limit of a few Gauss up to tens of kG. Our collaboration was the first to systematically study the magnetic fields in representative samples of different types of main-sequence B stars. In this article, we give an overview about what we have learned during the last years about magnetic fields in beta Cep, SPB, and Be stars.
http://hdl.handle.net/2268/156877
http://adsabs.harvard.edu/abs/2013arXiv1309.5497S
10 pages, 8 figures, 1 table, to appear in the Proceedings of the Conference: "Putting A Stars into Context: Evolution, Environment, and Related Stars"

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