VLT/SINFONI H₂ 1–0 S(1) intensity (left) and velocity (right) maps from Davies et al. (2006) showing a FoV similar to that of Fig. 5. The maps were derived by fitting a Gaussian to the emission line. The black dot marks the approximate location of the peak of the near-infrared continuum. The velocities are relative to this peak. To facilitate the comparison with the CO(2–1) and CO(3-2) emission, we show the same velocity range as in the right panels of Fig. 5.