Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-25T07:13:40.140Z Has data issue: false hasContentIssue false

The MiMeS project: magnetism in massive stars

Published online by Cambridge University Press:  01 November 2008

Gregg A. Wade
Affiliation:
Royal Military College of Canada
E. Alecian
Affiliation:
Royal Military College of Canada LESIA, France
D. A. Bohlender
Affiliation:
Canadian Astronomy Data Centre
J.-C. Bouret
Affiliation:
LAM, France
J. H. Grunhut
Affiliation:
Royal Military College of Canada
H. Henrichs
Affiliation:
Ast. Inst. Amsterdam, Netherlands
C. Neiner
Affiliation:
GEPI, France
V. Petit
Affiliation:
Université Laval, Canada
N. St. Louis
Affiliation:
Univ. de Montréal, Canada
M. Aurière
Affiliation:
LAT, France
O. Kochukhov
Affiliation:
Uppsala University, Sweden
J. Silvester
Affiliation:
Royal Military College of Canada
A. ud-Doula
Affiliation:
Morrisville State College, 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 is a consensus collaboration among the foremost international researchers of the physics of hot, massive stars, with the basic aim of understanding the origin, evolution and impact of magnetic fields in these objects. The cornerstone of the project is the MiMeS Large Program at the Canada-France-Hawaii Telescope, which represents a dedication of 640 hours of telescope time from 2008-2012. The MiMeS Large Program will exploit the unique capabilities of the ESPaDOnS spectropolarimeter to obtain critical missing information about the poorly-studied magnetic properties of these important stars, to confront current models and to guide theory.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Alecian, E., Wade, G. A., Catala, C., Bagnulo, S., et al. , 2008, A&A 481, 99Google Scholar
Alecian, E., Catala, C., Wade, G. A., Donati, J.-F., et al. , 2008, MNRAS 385, 391CrossRefGoogle Scholar
Arlt, R., 2008, Cont. Ast. Obs. Skalnaté Pleso, 38, p. 163Google Scholar
Auriere, M., Wade, G., Silvester, J., Lignières, F. et al. , 2007, A&A 475, 1053Google Scholar
Braithwaite, J., 2006, A&A 453, 687Google Scholar
Braithwaite, J., 2007, A&A 469, 275Google Scholar
Braithwaite, J. & Nordlund, A., 2006, A&A 450, 1077Google Scholar
Donati, J.-F., Semel, M., Carter, B. D., Rees, D. E., & Collier Cameron, A., 1997, MNRAS 291, 658CrossRefGoogle Scholar
Ferrario, L. & Wickramasinghe, D., 2006, MNRAS 367, 1323CrossRefGoogle Scholar
Kochukhov, O. & Piskunov, N., 2002, A&A 388, 868Google Scholar
Kochukhov, O., Bagnulo, S., Wade, G. A., Sangalli, L., et al. , 2004, A&A 414, 613Google Scholar
Kochukhov, O. & Bagnulo, S., 2006, A&A 450, 763Google Scholar
Mathys, G., Hubrig, S., Landstreet, J., Lanz, T., & Manfroid, J., 1997, A&AS 123, 353Google Scholar
Mestel, L., 1999, in Magnetic Fields Across the HR Diagram, ASP Conf. Proc. vol. 248, p. 3Google Scholar
Moss, D., 2001, Magnetic Fields Across the HR Diagram, ASP Conf. Proc. vol. 248, p. 305Google Scholar
Mullan, D. & MacDonald, J. 2005, MNRAS 356, 1139CrossRefGoogle Scholar
Petit, V., Wade, G. A., Drissen, L., Montmerle, T., & Alecian, E., 2008, MNRAS 387, 23CrossRefGoogle Scholar
Stone, J. & Norman, M., 1992, ApJS 80, 753CrossRefGoogle Scholar
Townsend, R. H. D., Owocki, S. P., & Ud-Doula, A., 2007, MNRAS 382, 139CrossRefGoogle Scholar
Wade, G. A., 2003, in Magnetic Fields in O, B and A Stars, ASP Conf. Proc. vol. 305, p. 16Google Scholar