Fig. 12
Left column: PACS/Spec continuum images (5 × 5 spatial array of 9′′ pixels regridded to a 1′′ grid) with contours of 37 μm (SOFIA) emission overlaid showing the positions of IRS 1, 2, and 3. Right column: top – total luminosity image with contours of fitted dust temperature at 70, 65, 60, ...K; center – luminosity image with contours of fitted dust optical depth at levels of 0.1, 0.15, 0.2, and 0.25; bottom – 450 μm SCUBA image with the same fitted dust optical depth contours overlaid.
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