Magnetic Fields in Galaxy Clusters and in the Large-Scale Structure of the Universe

被引：23

作者：

Vacca, Valentina ^{[1
]}

Murgia, Matteo ^{[1
]}

Govoni, Federica ^{[1
]}

Ensslin, Torsten ^{[2
]}

Oppermann, Niels ^{[3
]}

Feretti, Luigina ^{[4
]}

Giovannini, Gabriele ^{[4
,5
]}

Loi, Francesca ^{[5
]}

机构：

[1] INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargiu, Italy

[2] MPA, Karl Schwarzschild Str 1, D-85748 Garching, Germany

[3] Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada

[4] Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy

[5] Univ Bologna, Dept Phys Astron DIFA, Viale Berti Pichat 6-2, I-40126 Bologna, Italy

来源：

GALAXIES | 2018年 / 6卷 / 04期

关键词：

magnetic fields; acceleration of particles; polarization; statistics;

D O I：

10.3390/galaxies6040142

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The formation and history of cosmic magnetism is still widely unknown. Significant progress can be made through the study of magnetic fields properties in the large-scale structure of the Universe: galaxy clusters, filaments, and voids of the cosmic web. A powerful tool to study magnetization of these environments is represented by radio observations of diffuse synchrotron sources and background or embedded radio galaxies. To draw a detailed picture of cosmic magnetism, high-quality data of these sources need to be used in conjunction with sophisticated tools of analysis.

引用

页数：13

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