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Fig. 7


Comparison between the results from this work and those from Foyle et al. (2012) after reprojecting the dust properties in Foyle et al. (2012) to the common grid used in this work. The left panel compares the dust masses from the two studies, pixel by pixel. The right panel compares the average intensity of the interstellar radiation field (U) with the dust temperature (Tdust) derived by Foyle et al. (2012). Tdust has been related to U with the relationship (see text). The red dashed lines indicate the relationship when the quantities in horizontal and vertical axes are equivalent.

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