The magnetic characteristics of Galactic OB stars from the MiMeS survey of magnetism in massive stars

Authors
  • G.A. Wade
  • J. Grunhut
  • E. Alecian
  • C. Neiner
  • M. Aurière
  • D.A. Bohlender
  • A. David-Uraz
  • C. Folsom
  • H.F. Henrichs
  • O. Kochukhov
  • S. Mathis
  • S. Owocki
  • V. Petit
  • MiMes Collaboration
Publication date 2014
Journal Proceedings of the International Astronomical Union
Event Magnetic Fields throughout Stellar Evolution
Volume | Issue number 9 | S302
Pages (from-to) 265-269
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract The Magnetism in Massive Stars (MiMeS) project represents the largest systematic survey of stellar magnetism ever undertaken. Based on a sample of over 550 Galactic B and O-type stars, the MiMeS project has derived the basic characteristics of magnetism in hot, massive stars. Herein we report preliminary results.
Document type Article
Note In Volume 9, S302 (August 2013) © 2014. - Part of Symposium: Magnetic Fields throughout Stellar Evolution.
Language English
Published at
https://doi.org/10.1017/S1743921314002233 (Final published version)
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