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Fig. 15.


Kinetic power of the BLR winds as a function of the logarithm of the bolometric luminosities for the SUPER sample (diamonds). Values of the BLR winds from the WISSH sample (Vietri et al. 2018) (triangles) are also reported. The kinetic power of NLR winds from the SUPER sample is reported (gold shaded area). Kinetic power in fractions of 10−4, 10−5, and 10−6 bolometric luminosity are respectively indicated with dot-dashed, dashed, and dotted lines. BAL sources are denoted with red circles.

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