Outflow forces over bolometric luminosities for a sample of low-mass protostars, a sample of high-mass protostars, and extragalactic sources. Red points mark Class 0 low-mass protostars, with triangles taken from Yildiz et al. (2015) and circles from Mottram et al. (2017). Blue points mark Class I low-mass protostars, again with triangles from Yildiz et al. (2015), circles from Mottram et al. (2017), and stars from van der Marel et al. (2013). Gray squares mark the high-mass protostellar sample from Maud et al. (2015b) while gray crosses mark the intermediate mass sources described in van Kempen et al. (2009). The Cygnus-X sources, measured in this work, are shown with orange rectangles covering the extent of their outflow forces for the different available inclination correction factors. For the extragalactic sample, AGN sources are marked in magenta, with left-looking triangles for Seyfert I, right-looking triangles for Seyfert II and pentagons for LINER sources. Purple diamonds mark the starburst sources. Finally, filled points represent measurements taken from Lutz et al. (2020) and empty ones from Fluetsch et al. (2019).