MeerKAT view of the diffuse radio sources in Abell 3667 and their interactions with the thermal plasma

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Fig. 17.

Optical images from the Dark Energy Survey of two radio galaxies embedded into the emission of the SE radio relic. The contour levels in the top panel are (0.4, 0.8, 1.2, 1.6) × mJy beam⁻¹ with beam 10″ × 10″, and in the bottom panel they are (0.2, 0.3, 0.4, 0.525) × mJy beam⁻¹ with beam 10″ × 10″.

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