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Discussion – Winds and magnetic fields of active OB stars

Published online by Cambridge University Press:  12 July 2011

Jean-Claude Bouret  and
Lydia Cidale
Jean-Claude Bouret
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille Cedex 13, France NASA Goddard Space Flight Center, Greenbelt, 20771 MD, USA email: jean-claude.bouret@oamp.fr
Lydia Cidale
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata Instituto de Astrofísica La Plata, CCT La Plata-CONICET-UNLP Paseo del Bosque S/N, La Plata, Argentina email: lydia@fcaglp.unlp.edu.ar
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Abstract

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The discussion on winds and magnetic fields of active OB stars was carried out by S. Owoki, G. Wade, M. Cantiello, O. Kochukhov, M. Smith, C. Neiner, T. Rivinius, H. Henrichs and R. Townsend. The topics were the ability to detect small and large scale magnetic fields in massive stars and the need to consider limits on photometric variability of the star surface brightness.

Keywords

stars: early-typestars: magnetic fieldsstars: mass loss
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 172 - 175
Copyright
Copyright © International Astronomical Union 2011