Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales

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Fig. 5.

MeerKAT 1.283 GHz colour scale of the diffuse emission (same field as Fig. 3). The restoring beam is 40″ × 40″. The contours of the XMM-Newton surface brightness (see Sect. 3.4) are overlaid in white and are spaced by a factor of 2.

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