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

Published online by Cambridge University Press:  07 August 2014

G. A. Wade ,
J. Grunhut ,
E. Alecian ,
C. Neiner ,
M. Aurière ,
D. A. Bohlender ,
A. David-Uraz ,
C. Folsom ,
H. F. Henrichs  and
O. Kochukhov
...Show all authors
G. A. Wade
Affiliation:
RMC, Canada
J. Grunhut
Affiliation:
ESO, Germany
E. Alecian
Affiliation:
IPAG, France LESIA, France
C. Neiner
Affiliation:
LESIA, France
M. Aurière
Affiliation:
IRAP, France
D. A. Bohlender
Affiliation:
NRC, Canada
A. David-Uraz
Affiliation:
RMC, Canada
C. Folsom
Affiliation:
IRAP, France
H. F. Henrichs
Affiliation:
University of Amsterdam, Netherlands
O. Kochukhov
Affiliation:
Uppsala University, Sweden
S. Mathis
Affiliation:
LESIA, France CEA, France
S. Owocki
Affiliation:
University of Delaware, USA
V. Petit
Affiliation:
University of Delaware, USA
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Abstract

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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.

Keywords

Stars: early-typeStars: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 265 - 269
Copyright
Copyright © International Astronomical Union 2014 

References

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