Fig. 2
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Identified knots in the MUSE images. Left: the [O I]λ6300 (top) and [Fe II]λ7155 (bottom) emission lines with the tentative disk and halo noted in the [Ο II] panel. Emission is seen very close to the source, but whether this is the disk or the jet is undetermined. Right: the same images in grayscale, with the redshifted and blueshifted knots indicated by colored circles.
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