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

Open Access

Fig. 13.

Mini-halo injection in MS 0735.6+7421. Upper panels: MH injection in a close-by region void of sources. Lower panels: MH injection at cluster centre. First column: LOFAR image before the injection. Second column: Injection with r_e = 25 kpc. Third column: Injection with r_e = 50 kpc. Last column: Injection with r_e = 100 kpc.

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