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Fig. 6.

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Star-forming galaxies in the Ophiuchus cluster with detected radio emission. Each panel is 100 kpc × 100 kpc and shows the optical (Pan-STARRS, top) and optical/radio overlay (Pan-STARRS/MeerKAT, bottom). The first six galaxies show pronounced tails and are classified as jellyfish galaxies. In contrast, the last six galaxies do not show clear evidence of radio tails, either due to the presence of extended emission from the disk or contamination from the mini halo (see e.g. ID 106).

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