Fig. 10.
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Comparison between the CO(3−2) emission in the central 9″ × 9″ (left panel), with the Paα (middle) and H2λ2.12 μm (right) emission in the 8″ × 8″ FoV of the SINFONI observations (Busch et al. 2017). The CO contours are overlaid in the NIR images. The black star represents the AGN position listed in Table 1. Left panel: 15 regions are identified, R1–R11, I1–I3 and N, to compute the Kennicutt–Schmidt relation of Fig. 11.
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