Fig. 8.
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From left to right: MW, LMC, and SMC stars. Luminosity against mass-loss rate values for stars in our sample (black dots), Groenewegen (2022, red triangles), Groenewegen et al. (2009, blue pentagons), Groenewegen & Sloan (2018, green squares), and Riebel et al. (2012, purple crosses). The black point in the bottom right corner of each panel represents the average uncertainty of our estimated mass-loss rates for each galaxy.
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