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Fig. 8.


Fit of [O III], Hβ, [N II], Hα, and [S II] lines for two elements of the grid through which we divided the outfowing cones (see Fig. 7). The spectrum in panel a belongs to the SE blueshifted cone, the spectrum in panel b to the NW redshifted one. The blue Gaussian corresponds to the outflow kinematic component, the two green Gaussians (having the same velocity) to the disk; the velocity and velocity dispersion of all the Gaussians are tied between the lines. The purple vertical lines at [O III] and Hα wavelengths mark the stellar velocity for the element of the grid considered, obtained from the stellar kinematics presented in Fig. 6a. The reported wavelengths are in the Earth rest frame.

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