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Fig. 1.

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JWST/MRS emission line maps. From left to right: NGC 5506, NCG 5728 and NGC 7172. Top panels: 11.3 μm PAH feature intensity map. Central panels: H2 S(1) at 17.03 μm intensity map. Bottom panels: [Ne II] 12.81 μm intensity map. The black contours are the CO(3-2) emission from ALMA on a logarithmic scale. The first and last contours lie at 3σ and the peak flux, respectively. North is up and east is to the left, and offsets are measured relative to the AGN. Orange solid circle and white ellipse correspond to the JWST and ALMA beams, respectively.

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