The MiMeS project: magnetism in massive stars

被引：10

作者：

Wade, Gregg A. ^{[1
]}

Alecian, E. ^{[1
,2
]}

Bohlender, D. A. ^{[3
]}

Bouret, J. -C. ^{[4
]}

Grunhut, J. H. ^{[1
]}

Henrichs, H. ^{[5
]}

Neiner, C. ^{[6
]}

Petit, V. ^{[7
]}

St Louis, N. ^{[8
]}

Auriere, M. ^{[9
]}

Kochukhov, O. ^{[10
]}

Silvester, J. ^{[1
]}

ud-Doula, A. ^{[11
]}

机构：

[1] Royal Mil Coll Canada, Kingston, ON, Canada

[2] LESIA, Meudon, France

[3] Canadian Astron Data Ctr, Victoria, BC, Canada

[4] LAM, Marseille, France

[5] Ast Inst, Amsterdam, Netherlands

[6] GEPI, Meudon, France

[7] Univ Laval, Laval, PQ, Canada

[8] Univ Montreal, Montreal, PQ, Canada

[9] LAT, Paris, France

[10] Uppsala Univ, Uppsala, Sweden

[11] Morrisville State Coll, Morrisville, NY USA

来源：

COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES | 2009年 / 259期

关键词：

Magnetic fields; massive stars; hot stars; star formation; stellar evolution; stellar winds; spectropolarimetry; FIELDS; STABILITY; AP;

D O I：

10.1017/S1743921309030695

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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.

引用

页码：333 / +

页数：2

共 20 条

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