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Fig. 2


Hi-GAL 250 μm emission (contours) of the G29-SFR cloud overlaid on the 13CO (1–0) emission (grayscale) from GRS averaged over the 95–105 km s-1 velocity interval. Contour levels are 7, 9, 14, 18, 24, 36, 48, 72, and 96% of the peak of the 250 μm emission, 36 311 MJy/sr. Grayscale levels are 10, 15, 20, 40, 60, 80, and 100% of the peak of the 13CO emission, 5 K. The crosses indicate the positions of the Hi-GAL sources associated with the cloud detected in the 5 Hi-GAL photometric bands. Red and green crosses indicate, respectively, sources associated and non-associated with Spitzer 24 μm emission. The white cross marks the position of the Hi-GAL source associated with the G29-UC region and G29-HMC core (see Sect. 3.2), which is also associated with 24 μm emission.

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