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

Journal
Date Issued
2018
Author(s)
•
•
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Enßlin, Torsten
•
Oppermann, Niels
•
•
•
DOI
Abstract
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.
Volume
6
Issue
4
Start page
142
Uri
Url
Issn Identifier
2075-4434
Ads BibCode
2018Galax...6..142V
Rights
open.access
File(s)
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4.68 MB

Format

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