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Fig. 2

image

Left panel: AGN bolometric luminosity as a function of the maximum wind velocity, vmax. The black dashed lines mark a scaling. The magenta solid line is the best fit correlation found by Spoon et al. (2013) for OH outflows. The two cyan solid lines are the best fit scaling found by Veilleux et al. (2013) for OH outflows, using vmax and v80. The cyan boxes and filled dot are the loci covered by two groups of Swift BAT AGN with 42.3 < Lbol < 43.3 and 43.7 < Lbol < 44.3 and by the outlier NGC 7479, from Stone et al. (2016). Right panel: wind momentum load (outflow momentum rate divided by the AGN radiation momentum rate L/c) as a function of vmax. The red dashed line mark the expectations for a momentum conserving outflow. The two blue solid lines mark the expectations for pure energy conserving outflows for Markarian 231 (starred circle) and IRAS F11119+13257 (squared circle). Symbols as in Fig. 1.

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