Fig. 2.
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Properties of the gas outflows. The color code shows the dependence of the fraction of cold gas that is expelled by AGN outflows (fexpell, top panel) and of the solid angle θc swept out by AGN outflows (bottom panel) on the AGN bolometric luminosity LAGN and of the cold gas mass Mcold. A DM circular velocity Vc = 200 km s−1 is assumed for both panels.
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