Fig. 2.
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Colour-coding for both figures is on evolutionary stage, legend shown in panel a. These plots show the sample of 17 quiescent, 23 protostellar, 22 YSO, and 25 HII regions. (a) Stacked histogram distribution of the luminosity-to-mass ratio for the regions in the ALMAGAL sub-sample being used for this work. (b) Individual cumulative distribution functions (CDF) of regions in each evolutionary stage, generated from kernel density estimates (KDEs) of the data shown in (a).
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