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Fig. 3.

image

Radial variation of properties in the disc of the MaNGA galaxy M-7495-12704 with the circumnuclear region of the AGN type (Fig. 2). Panels show the surface brightness in Hα (panel a) and [O III]λλ4959,5007 (panel b) lines, the observed (non corrected for instrumental profile) velocity dispersion of the gas σgas, obs (panel c) and stars σstar, obs (panel d), the coordinates in the BPT diagram XBPT = log([N II]λ6584/Hα) (panel e), and YBPT = log([O III]λ5007/Hβ) (panel f), as a function of the galactocentric distance. The BPT type of the spectra is color-coded. The spaxels classified as intermediate-type in the disc and in the circumnuclear region (center) are shown by different colors.

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