First evidence of a connection between cluster-scale diffuse radio emission in cool-core galaxy clusters and sloshing features

Open Access

Fig. 16.

A1204 cavity detection. Left panel: Chandra X-ray image smoothed on a scale of 1″. Central panel: Residual image after the subtraction of a circular β-model. Right panel: Residual image after the subtraction of a circular double β-model. In all the panels, green circles indicate the position of the cavities.

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