Magnetic fields in the galactic Universe, as observed in supershells, galaxies, intergalactic and cosmic realms

被引:56
|
作者
Vallee, Jacques P. [1 ]
机构
[1] Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7, Canada
关键词
SAGITTARIUS-A-ASTERISK; LINEAR-POLARIZATION OBSERVATIONS; FARADAY-ROTATION MEASURES; RADIO-CONTINUUM EMISSION; LARGE-SCALE STRUCTURE; GAMMA-RAY BURST; MICROWAVE BACKGROUND POLARIZATION; NEUTRAL HYDROGEN DISTRIBUTIONS; ZEEMAN-EFFECT OBSERVATIONS; LARGE ARRAY OBSERVATIONS;
D O I
10.1016/j.newar.2011.01.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Here I present a survey of magnetic fields in large objects, from the interstellar supershells (10 pc) up to the edge of the Universe (near a redshift z of 10), with an emphasis on discoveries made in the last decade, be they through particle astronomy or electromagnetic astronomy. For each type of object, the basic observational properties are summarized, and the best theoretical scenario which accounts for the large body of observations is discussed. The strength of these large-scale fields can vary from mGauss to mu Gauss. Magnetism acts as a tracer of the dynamical histories of cosmological and intracluster events, it guides the motion of the interstellar ionised gas, and it aligns the charged dust particles. Crown Copyright (C) 2011 Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:91 / 154
页数:64
相关论文
共 50 条