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Radio Halos in Merging Clusters
Published online by Cambridge University Press: 30 March 2016
Abstract
The number of known diffuse radio sources in clusters of galaxies (halos and relics) has grown in recent years, making it possible to derive statistical considerations on the physical conditions of these sources and on the properties of related clusters. We will discuss the percentage of clusters with a diffuse source and will show evidence that diffuse sources are associated with X-ray luminous clusters which have undergone recent merger processes.
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- Copyright © Astronomical Society of Pacific 2002
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