Fig. 6
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Dust temperatures (upper panel) and masses (lower panel) of clumps in the Lagoon Nebula. The circle size corresponds to the aperture size used for flux extraction in the analysis. For the temperatures, the smaller inner circles visualise the derived temperatures of the hot components. The grey-scale background image shows the JCMT SCUBA 870 µm dust continuum flux (see Fig. 2).
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