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Fig. 3.

image

Left panels: ionized gas velocity and velocity dispersion maps (upper panels) for HE 0227–0913 together with the Hα and [O III] surface brightness maps from the MUSE data after stellar continuum subtraction. Contours of the continuum emission are in logarithmic scaling are overlayed in gray. Right panels: emission-line diagnostic diagram for spaxels with a S/N >  3 in each line (upper panel). Excitation map after separating line ratios, into star forming, AGN, intermediate and LINER-like ionization.

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