Outflow momentum rate plotted against its velocity for twelve objects with both ultra-fast winds and large-scale galactic outflows, adapted from Smith et al. (2019). Different colors and shapes identify different objects and outflows. Solid error bars are used for values with upper and lower errors calculated, dotted bars if only a range of value was available, and arrows for limits. Values reported in this plot taken from this work, Bischetti et al. (2019), Chartas et al. (2020), Cicone et al. (2014), Feruglio et al. (2015, 2017), Fluetsch et al. (2019), García-Burillo et al. (2014), González-Alfonso et al. (2017), Luminari et al. (2018), Longinotti et al. (2018), Marasco et al. (2020), Mizumoto et al. (2019), Longinotti et al. (2015), Rupke et al. (2017), Sirressi et al. (2019), Smith et al. (2019), Tombesi et al. (2015, 2017), Tozzi et al. (2021), Veilleux et al. (2017).