The MiMeS Project: Magnetism in Massive Stars
arXiv:0812.4078 · doi:10.1017/S1743921309030695
Abstract
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.
6 pages, 3 figures, proceedings of IAUS 259: Cosmic Magnetic Fields
References in corpus (5)
- Characterisation of the magnetic field of the Herbig Be star HD 200775
- A Rigid-Field Hydrodynamics approach to modeling the magnetospheres of massive stars
- The stability of poloidal magnetic fields in rotating stars
- Discovery of two magnetic massive stars in the Orion Nebula Cluster: a clue to the origin of neutron star magnetic fields?
- Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)