Fig. 12
Zoom into the column density maps of NGC 3603, Carina, and Auriga where we determined the column density profiles shown in Fig. 13. Lower right panel: a temperature map of NGC 3603. The white, dashed circle includes all the pixels we included for the profile and the black, dashed circles for NGC 3603 and Carina outline the area where we observe a possible slope change in the column density profile.
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