Fig. 11
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Left: kinetic luminosity of BCG radio galaxies estimated at 1.4 GHz vs. X-ray luminosity of the host cluster or group for the eFEDS sample. Data are classified into non-cool cores (red), moderately cool cores (blue), and cool cores (black) based on the concentration parameter. Right: same as in the left panel, with data classified based on the Rscore (see discussion).
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