Non-thermal emission in galaxy groups at extremely low frequency: The case of A1213

Open Access

Fig. 5.

X-ray map of A1213 with overlaid radio contours. Left: LOFAR 54 MHz contours (green) overlaid on the XMM-Newton map in the energy range 0.7−1.2 keV. R₂₀₀ is ∼1140 kpc, which lies outside of our field of view. Right: Zoom on 4C 29.41 contours as detected at 144 MHz from the 0.3″ resolution image, overlaid on the same XMM-Newton map shown on the left panel.

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