Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T16:42:19.112Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Alecian, E., Kochukhov, O., Neiner, C., Wade, G. A.et al., 2011, A&A, 536, 6Google Scholar
Briquet, M., Neiner, C., Leroy, B., & Pápics, P. I., 2013, A&A, 557, 16Google Scholar
Donati, J.-F., Semel, M., Carter, B. D., Rees, D. E., et al., 1997, MNRAS, 291, 658CrossRefGoogle Scholar
Grunhut, J., Wade, G. A., Marcolino, W., Petit, V.et al., 2009, MNRAS, 400, 94Google Scholar
Kochukhov, O., Makaganiuk, V., & Piskunov, N., 2010, A&A, 524, 5Google Scholar
Mestel, L. 1999, in Magnetic Fields Across the HR Diagram, ASP Conf. Proc. Vol. 248, 3Google Scholar
Neiner, C., Grunhut, J., Petit, V., ud-Doula, A., A et al., 2012, MNRAS, 426, 2738Google Scholar
Petit, V., Wade, G. A., Drissen, L., Montmerle, T., & Alecian, E., 2008, MNRAS, 387, 23Google Scholar
Petit, V. & Wade, G. A., 2012, MNRAS, 420, 73CrossRefGoogle Scholar
Silvester, J., Kochukhov, O. & Wade, G. A., 2013, MNRAS, submittedGoogle Scholar
Shultz, M., Wade, G. A., Grunhut, J., Bagnulo, S.et al., ApJ 750, 2CrossRefGoogle Scholar
Sundqvist, J., ud-Doula, A., Owocki, S., Townsend, R., et al., 2012, MNRAS, 423, 21Google Scholar
Wade, G. A., Maíz Apellániz, J., Martins, F., Petit, V., et al., 2012, MNRAS, 425, 1278CrossRefGoogle Scholar