Fig. 3.
Component of sources 𝒮λ that is composed of the images of radiative transfer models of 828 starless and 91 protostellar cores and convolved to the Herschel resolutions Oλ (cf. Sect. 1), shown at three selected wavelengths. Only the bright unresolved emission peaks of the protostellar cores, clearly visible at 100 μm, appear in the 70 μm image (not shown). Square-root color mapping.
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