[en] The magnetic activity of solar-type and low-mass stars is a well known source of coronal X-ray emission. At the other end of the main sequence, X-rays emission is instead associated with the powerful, radiatively driven winds of massive stars. Indeed, the intrinsically unstable line-driving mechanism of OB star winds gives rise to shock-heated, soft emission (~0.5 keV) distributed throughout the wind. Recently, the latest generation of spectropolarimetric instrumentation has uncovered a population of massive OB-stars hosting strong, organized magnetic fields. The magnetic characteristics of these stars are similar to the apparently fossil magnetic fields of the chemically peculiar ApBp stars. Magnetic channeling of these OB stars' strong winds leads to the formation of large-scale shock-heated magnetospheres, which can modify UV resonance lines, create complex distributions of cooled Halpha emitting material, and radiate hard (~2-5 keV) X-rays. This presentation summarizes our coordinated observational and modelling efforts to characterize the manifestation of these magnetospheres in the X-ray domain, providing an important contrast between the emission originating in shocks associated with the large-scale fossil fields of massive stars, and the X-rays associated with the activity of complex, dynamo-generated fields in lower-mass stars.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Petit, V.; Dept. of Physics & Astronomy, University of Delaware, Newark, DE, USA
Cohen, D. H.; Dept. of Physics & Astronomy, Swarthmore College, Swarthmore, PA, USA
Nazé, Yaël ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Gagné, M.; Dept. of Geology & Astronomy, West Chester University, West Chester, PA, USA
Townsend, R. H. D.; Dept. of Astronomy, University of Wisconsin-Madison, Madison, WI, USA
Leutenegger, M. A.; Laboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD, USA
ud-Doula, A.; Penn State Worthington Scranton, Dunmore, PA, USA
Owocki, S. P.; Dept. of Physics & Astronomy, University of Delaware, Newark, DE, USA
Wade, G. A.; Dept. of Physics, Royal Military College of Canada, Kingston, ON, Canada)
Language :
English
Title :
X-rays from magnetic massive OB stars
Publication date :
01 August 2014
Event name :
IAUS 302: Magnetic fields throughout stellar evolution
Event place :
Biarritz, France
Event date :
25-28 August 2013
Audience :
International
Journal title :
Proceedings of the International Astronomical Union
ISSN :
1743-9213
eISSN :
1743-9221
Publisher :
Cambridge University Press, Cambridge, United Kingdom
