All Mixed Up - Relations between Cluster Thermal and Non-Thermal Plasmas

Physics

Scientific paper

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Scientific paper

I report on explorations of the spatial and physical relationships between cluster thermal and relativistic plasmas. In Coma, we find a large shock-like structure bordering the radio halo which led to its recovery in X-rays. However, the overall structure of the radio halo is not well matched to the diffuse X-rays, suggesting multiple energization sources. New EVLA observations of A2256 using RM synthesis allows us to start probing its line of sight structure -- tailed radio galaxies show local Faraday effects, confusing estimates of the cluster-wide fields. Numerical simulations show how these AGNs interact with the cluster weather. Finally, we constrain the relativistic plasma energization in X-ray clusters using a radio stacking experiment.

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