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Fig. 3


Left panel: outflow kinetic power as a function of the star formation rate in the host galaxy (computed, when possible, in a region similar to that where the outflow has been detected). The dashed line is the expectation of a SN-driven wind, by assuming 0.0066 SNe per solar mass of newly formed star (Salpeter IMF) a total luminosity for each SN of 1051 erg/s and an efficiency of releasing this luminosity in the ISM to drive a shock of 10%. The solid red line is the expected SFR obtained using the Netzer (2009) relationship between SFR and AGN bolometric luminosity and assuming the average Ėkin/Lbol = 0.025 found for molecular winds in Fig. 1. Right panel: AGN bolometric luminosity as a function of the host galaxy star formation rate. The red, magenta and cyan lines in the right panel are the expected relations based on the SFRLbol correlations by Netzer (2009), Hickox et al. (2014; z = 0) and Hickox et al. (2014, z = 2), respectively. Symbols as in Fig. 1.

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