Fig. 10.

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Spaxel-by-spaxel plot of the ratio between the H2 0–0 S(1) luminosity and the monochromatic continuum luminosity νLν at 17 μm (with Lν spectral luminosity). The ratio increases with the projected distance from the AGN up to 30 pc, pointing at a stronger non-radiative excitation of H2 in the outer parts of the ICND. The horizontal dashed line indicates the UV PDR limit from Guillard et al. (2012b) rescaled using the LPAH7.7μm/L17μm ratio of the PAH7.7μm and the continuum at 17 μm (averaged over the ICND).
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