Fig. B.1
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Upper panel: Comparison of the flux density extracted inside a 40.9″ beam for the AKARI and PACS images of selected clumps in NGC 6334. Lower panel: Luminosities of these clumps as derived from fitting SEDs with the AKARI data as compared to the luminosities derived by Urquhart et al. (2018) for the same clumps. The fitted linear relation and the Pearson correlation coefficient R and the P value are given in the upper-left corner.
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