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MiMeS项目：大质量恒星的磁性

The MiMeS Project: Magnetism in Massive Stars

G. A. Wade, E. Alecian, D. A. Bohlender, J. -C. Bouret, J. H. Grunhut, H. Henrichs, C. Neiner, V. Petit, N. St. Louis, M. Auriere, O. Kochukhov, J. Silvester, A… 展开作者

G. A. Wade, E. Alecian, D. A. Bohlender, J. -C. Bouret, J. H. Grunhut, H. Henrichs, C. Neiner, V. Petit, N. St. Louis, M. Auriere, O. Kochukhov, J. Silvester, A. ud-Doula, the MiMeS Collaboration

备注：
6 pages, 3 figures, proceedings of IAUS 259: Cosmic Magnetic Fields
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摘要：

大质量恒星中的磁性（MiMeS）项目是国际上最重要的热、大质量恒星物理学研究人员之间的共识合作，其基本目的是了解这些物体中磁场的起源、演变和影响。该项目的基石是加拿大-法国-夏威夷望远镜的MiMeS大型计划，该计划代表了2008-2012年640小时的望远镜时间。MiMeS大型计划将利用ESPaDOnS分光偏振仪的独特功能，获得有关这些重要恒星的磁特性研究不足的关键缺失信息，以对抗当前模型并指导理论。

英文摘要：

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.

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