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Fig. 2


Left: star forming ATLASGAL clump, AGAL007.166+00.131, associated with a MIPSGAL selected YSO. The background image is the MIPSGAL 24 μm image, the contours show the masked 870 μm intensity. The YSO is located at the peak of the dust emission. Right: quiescent clump, AGAL022.531-00.192. The faint 24 μm source projected onto the dust emission is not identified as a YSO.

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