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Fig. 1


Left panel: the wind mass outflow rate as a function of the AGN bolometric luminosity. AGN for which molecular winds have been reported in the literature (mostly local ULIRGs and Seyfert galaxies) are shown with blue symbols. In particular: open circles are CO outflows; the open square is the measurement for IRAS 23060; filled squares are OH outflows; the starred open circles are for Markarian 231 (large symbol for the outflow measured within ROF = 1 kpc and small symbol for the outflow at ROF = 0.3 kpc); the crossed open circles are the measurements for NGC 6240 (large symbol for ROF = 3.5 kpc and small symbol for ROF = 0.6 kpc); the small dotted open triangle marks the measurement in the circum nuclear disk of NGC 1068 (ROF = 0.1 kpc) and NGC 1433 (ROF = 0.06 kpc); the small dotted open circles represent the measurements for NGC 1266, IC 5066 at ROF = 0.5 kpc; the squared open circle marks IRAS F11119+13257 measurement at ROF = 0.3 kpc. Green symbols mark ionised outflows measurements. In details: filled squares mark z> 1 AGN; filled triangles mark z = 0.1–0.2 AGN; open triangles mark z = 0.4–0.6 type 2 AGN; pentagons mark z = 2–3 radiogalaxies; filled circles mark hyper-luminous z = 2–3 QSOs. BAL winds are shown with black stars. The black open pentagon highlights the [CII] wind in J1148+5251 at z = 6.4. Finally, red symbols mark X-ray outflows. In details: large five pointed stars are local UFOs; the starred open circle, the filled triangle and the circled square are the measurement for Markarian 231, PDS456 and IRAS F11119+13257, respectively. Small five point stars are slower warm absorbers. The dashed blue, green and red lines are the best fit correlations of the molecular, ionised, and X-ray absorber samples, respectively. Right panel: wind kinetic power as a function of the AGN bolometric luminosity. Solid, dashed and dotted line represent the correlations Ėkin = 1,0.1,0.01 Lbol.

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