Deep Chandra data confirms three cold fronts in RXJ2014.8-2430 with widths indicating suppressed diffusion and identifies a concave structure consistent with either a Kelvin-Helmholtz instability or a powerful AGN cavity of radius 200-330 kpc.
Planck Collaboration et al.A&A, 594:A22, Sept
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MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.
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A Detailed View of the Large-Scale Sloshing Cold Front in RXJ2014.8-2430
Deep Chandra data confirms three cold fronts in RXJ2014.8-2430 with widths indicating suppressed diffusion and identifies a concave structure consistent with either a Kelvin-Helmholtz instability or a powerful AGN cavity of radius 200-330 kpc.
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Study of Polarized Emission in Radio Halos and Filaments in the SKA Telescopes Era
MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.