Fig. 6.

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PVDs of the S(1) line. Left panels: Flux and velocity dispersion maps obtained using bilinear interpolation, with the regions used to extract the PVDs superimposed, which have a size of 06 × 7″. Middle and right panels: PVDs extracted along the kinematic major and minor axes determined by 3DBAROLO (top) and along PA = 87° and 3° (bottom). The black and magenta contours correspond to the data and rotating disk model above 2σ (see Sect. 3.2.3). The high-velocity emissions observed between –1 and 1 arcsec correspond to artifacts in the nuclear region because of the strong AGN continuum and derived low EW of the molecular emission lines there.
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