Fig. 10.

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Comparison of the outflow properties with the bolometric luminosity of the AGN (Lbol) and the Eddington ratio (Lbol/Ledd). Left panel: total kinetic energy of the outflow vs. Lbol. These quantities show a linear dependence. Right panel: velocity of the outflow vs. Lbol/Ledd. Most sources show velocities between ∼200 and ∼800 km s−1 with no clear trend with Lbol/Ledd or differences between the various spectroscopic classes. The open symbols correspond to sources without detected extended outflow.
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