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- W2904159842 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." @default.
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- W2904159842 date "2018-12-17" @default.
- W2904159842 modified "2023-09-24" @default.
- W2904159842 title "Magnetic Fields in Galaxy Clusters and in the Large-Scale Structure of the Universe" @default.
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- W2904159842 doi "https://doi.org/10.3390/galaxies6040142" @default.
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