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Fig. 3

image

Distribution of the SABOCA continuum emission at 350 μm along the infrared dark cloud in G327.3–0.6. Contours are from 5% of the peak flux in steps of 10%. The triangles mark the positions of the submillimeter continuum peaks reported in Table 3. The red cross marks the position observed for the single pointing HIFI observations. The white circle in the bottom left corner shows the beam of the SABOCA observations.

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