Fig. 6.

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Schematic view of the atomic and molecular absorptions. The HST legacy archive image of the absorbing galaxy in H-band (F160W) is plotted on the left, and the 5 GHz VLBI image from Perlman et al. (1996) showing the jet (west) and counterjet (east) is on the right. The contours are spaced by a factor of in brightness. The component N is the nucleus or radio core. The counterjet components are indicated by A, B, and C. The HI absorption is centered in B, and the molecular components in N. The jet structure is aligned on the minor axis of the galaxy.
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