Turning AGN Bubbles into Radio Relics with Sloshing: Modeling CR Transport with Realistic Physics
@article{ZuHone2021TurningAB, title={Turning AGN Bubbles into Radio Relics with Sloshing: Modeling CR Transport with Realistic Physics}, author={John A. ZuHone and K Ehlert and Rainer Weinberger and Christoph Pfrommer}, journal={Galaxies}, year={2021} }
Radio relics are arc-like synchrotron sources at the periphery of galaxy clusters, produced by cosmic-ray electrons in a μG magnetic field, which are believed to have been (re-)accelerated by merger shock fronts. However, not all relics appear at the same location as shocks as seen in the X-ray. In a previous work, we suggested that the shape of some relics may result from the pre-existing spatial distribution of cosmic-ray electrons, and tested this hypothesis using simulations by launching…
2 Citations
The Merger Dynamics of the X-ray Emitting Plasma in Clusters of Galaxies
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As the formation of cosmic structure continues to proceed, we observe one of the latest stages of this process in mergers of clusters of galaxies with other clusters, groups, and galaxies. The X-ray…
New Window on the Radio Emission from Galaxies, Clusters and Cosmic Web—Conference Summary
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This manuscript summarizes the contributions presented and discussed during the conference “A new window on radio galaxies, clusters and cosmic web: current status and new challenges”. The meeting…
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