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Fig. 9

image

OSIRIS Hα (left) and CALIFA Hα (right) emission line fluxes in units of 10-16 erg s-1 cm-2 arcsec-2 presented on a logarithmic scale. The black cone delimits the nuclear outflowing nebula reported by Lípari et al. (2004). The HST F555W image is shown in contours, smoothed to approximately match the spatial resolution of our IFS data.

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