2014MNRAS.441L..31W

We search the cool core galaxy clusters in the REXCESS sample for evidence of large-scale gas sloshing, and find clear evidence for sloshing in RXJ2014.8-2430, the strongest cool core cluster in the REXCESS cluster sample. The residuals of the surface brightness distribution from the azimuthal average for RXJ2014 show a prominent swirling excess feature extending out to an abrupt surface brightness discontinuity at 800kpc from the cluster core (half the virial radius) to the south, which the XMM-Newton observations confirm to be cold, low-entropy gas. The gas temperature is significantly higher outside this southern surface brightness discontinuity, indicating that this is a cold front 800kpc from the cluster core. Chandra observations of the central 200kpc show two clear younger cold fronts on opposite sides of the cluster. The scenario appears qualitatively consistent with simulations of gas sloshing due to minor mergers which raise cold, low-entropy gas from the core to higher radius, resulting in a swirling distribution of opposing cold fronts at increasing radii. However, the scale of the observed sloshing is much larger than that which has been simulated at present, and is similar to the large-scale sloshing recently observed in the Perseus cluster and Abell 2142.