Fig. 10.

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Slope of the power-law fits performed to the log M* − log Mdisk (top panel) and log Mdisk − log Ṁacc (bottom panel) relationships for the four regions studied in this work. The circles represent the slopes of the power-law fit performed to the entire data set, and the stars that performed to the stellar population. A small offset in age in the slopes of each region was performed for visualization purposes. The symbols follow the same color-coding as in Fig. 5.
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