Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-05T00:47:13.195Z Has data issue: false hasContentIssue false
  • English
  • Français

The MiMeS project: overview and current status

Published online by Cambridge University Press:  12 July 2011

Gregg A. Wade ,
Evelyne Alecian ,
David A. Bohlender ,
Jean-Claude Bouret ,
David H. Cohen ,
Vincent Duez ,
Marc Gagné ,
Jason H. Grunhut ,
Huib F. Henrichs  and
Nick R. Hill
...Show all authors
Gregg A. Wade
Affiliation:
Kingston, Canada
Evelyne Alecian
Affiliation:
LOAG, France
David A. Bohlender
Affiliation:
HIA, Canada
Jean-Claude Bouret
Affiliation:
LAM, France
David H. Cohen
Affiliation:
Swarthmore, USA
Vincent Duez
Affiliation:
Argelander, Germany
Marc Gagné
Affiliation:
West Chester, USA
Jason H. Grunhut
Affiliation:
Kingston, Canada
Huib F. Henrichs
Affiliation:
Amsterdam, Netherlands
Nick R. Hill
Affiliation:
Madison, USA
Oleg Kochukhov
Affiliation:
Uppsala, Sweden
Stéphane Mathis
Affiliation:
CEA, France
Coralie Neiner
Affiliation:
Paris Observatory, France
Mary E. Oksala
Affiliation:
Delaware, USA
Stan Owocki
Affiliation:
Delaware, USA
Véronique Petit
Affiliation:
West Chester, USA
Matthew Shultz
Affiliation:
Kingston, Canada
Thomas Rivinius
Affiliation:
ESO, Chile
Richard H. D. Townsend
Affiliation:
Madison, USA
Jorick S. Vink
Affiliation:
Armagh, UK
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 many of 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. At the time of writing, MiMeS Large Programs have acquired over 950 high-resolution polarised spectra of about 150 individual stars with spectral types from B5-O4, discovering new magnetic fields in a dozen hot, massive stars. The quality of this spectral and magnetic matériel is very high, and the Collaboration is keen to connect with colleagues capable of exploiting the data in new or unforeseen ways. In this paper we review the structure of the MiMeS observing programs and report the status of observations, data modeling and development of related theory.

Keywords

stars: magnetic fieldsstars: early-typestars: formationstars: evolutionstars: windsoutflowstechniques: polarimetric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 118 - 123
Copyright
Copyright © International Astronomical Union 2011

References

Alecian, E., Catala, C., Wade, G. A., Donati, J.-F. et al. 2008, MNRAS, 385, 391Google Scholar
Arlt, R. 2008, Contributions of the Astronomical Observatory Skalnate Pleso 38, 163Google Scholar
Braithwaite, J. 2006, A&A 453, 687Google Scholar
Braithwaite, J. 2007, A&A 469, 275Google Scholar
Donati, J.-F., Semel, M., Carter, B. D., Rees, D. E. et al. 1997, MNRAS 291, 658CrossRefGoogle Scholar
Donati, J.-F., Howarth, I. D., Jardine, M. M., Petit, P. et al. 2006, MNRAS 370, 629Google Scholar
Duez, V. & Mathis, S. 2010, A&A 517A, 58Google Scholar
Kochukhov, O., Bagnulo, S., Wade, G. A., Sangalli, L. et al. 2004, A&A 414, 613Google Scholar
Kochukhov, O. & Wade, G. A. 2010, A&A 513A, 13Google Scholar
Petit, V., Wade, G. A., Drissen, L., Montmerle, T. et al. 2008, MNRAS 387, L23CrossRefGoogle Scholar
Piskunov, N. & Kochukhov, O. 2002, A&A 381, 736Google Scholar
Stone, J. M. & Norman, M. L. 1992, ApJS 80, 753Google Scholar
Townsend, R. H. D., Owocki, S. P., & Ud-Doula, A. 2007, MNRAS 382, 139CrossRefGoogle Scholar
ud-Doula, A., Owocki, S. P., & Townsend, R. H. D. 2008, MNRAS 385, 97Google Scholar