Wind vs. driving mechanism energetics for local galaxies with massive molecular wind detections. A: wind momentum rate vs. radiation pressure of AGN photons. B: wind kinetic luminosity vs. jet power. The dashed lines indicate different ratios of the plotted parameters. C: outflow’s momentum rate relation with the total photon momentum output of the galaxy. The dashed lines denote the different values of the ratio of outflow’s momentum rate over bolometric luminosity. The arrows denote upper limit values.