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Fig. 3


Total-power contours of radio emission without nearby background sources for NGC 4605 at 4.85 GHz a) and NGC 5204 at 8.35 GHz b). The contour levels and other map parameters are the same as in Figs. 1 and 2. The positions of the subtracted background sources are marked by asterisks.

This figure is made of several images, please see below:

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