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Fig. 3.

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Flux [ × 10−20 erg s−1 cm−2] (left), velocity [km/s] (center), and velocity dispersion [km/s] (right) maps of the different H2 rotational transitions detected in the MIRI/MRS data. The magenta contours represent 10%, 20%, 30%, 40%, 50%, 60%, 70%, 80%, and 90% of the maximum ALMA CO(2−1) flux. For the S(1), S(2), and S(3) maps we also included the ALMA contours corresponding to 7% and 8% of the maximum flux. The black contours correspond to the 5%, 10%, 15%, and 20% of the average σ (∼2.85 × 10−5) in the VLA 8.4 GHz image. The white star shows the AGN location according to the ALMA continuum. The VLA and ALMA beams, corresponding to 0 . $ \overset{\prime \prime }{.} $14 × 0 . $ \overset{\prime \prime }{.} $30 and 0 . $ \overset{\prime \prime }{.} $68 × 0 . $ \overset{\prime \prime }{.} $83, are shown in the S(1) and S(5) flux maps.

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