Upper left: composite image (LABOCA 870 μm, Spitzer 3.6 and 8.0 μm) of the giant pillar in the Southern Pillars region (box “b” in Fig. 1 and 2). Temperature map (upper right), Column density map, expressed in cm-2 (lower left) and FUV flux G0 (in units of the Habing field) (lower right) of the enlargement of the region. The solid lines highlight the cut lines of the prominent pillars for which temperature and column density are shown in Fig. 6.
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