Fig. 3
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Radial profiles of selected cuts in three fibers belonging to the Flame Nebula (left panel), LDN 1641N (central panel), and NGC 2023 (right panel). Similarly to Fig. 2, we report the distance at which the temperature gradient is determined (dashed black lines) and the FWHMs determined from the best Gaussian fit (solid black line) to the density profile (blue line).
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