AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 5506

Open Access

Fig. 14.

Radial profiles for the different mean velocities of the [OIII] line, all as a function of the projected distance from the AGN. Panels show, from top to bottom: the rotational velocity v_rot along the kinematic axis, the broad velocity Δv, the 80% width W₈₀, and our estimate for the mean outflow velocity of the ionised gas $v_{out}^{ion}$ $v_{\mathrm{out}}^{\mathrm{ion}}$ .

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