Open Access
Fig. 9
Herschel images of W48: a) PACS 70 μm (HPBW ~ 6); b) PACS 160 μm (HPBW ~ 12); c) SPIRE 250 μm (HPBW ~ 18); d) SPIRE 350 μm (HPBW ~ 25); and e) SPIRE 500 μm (HPBW37). The bright diffuse emission on the right of each panel is from the Galactic plane. Plus signs (+) indicate the location of supernova remnants.
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