Fig. 9
Dust emission: MIPS 24 μm, HiGAL 70, 250, 350, and 500 μm photometric data, all convolved to 42″ resolution (squares, with an intensity uncertainty of ≲15%). Continuous curves show the best-fit BG SEDs of representative positions A, B, C, and D. The 24 μm emissionis produced by hotter VSGs. The area below the continuous curves (40–500 μm) is the integrated FIR intensity (IFIR).
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