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Fig. 8


Dust continuum emission maps for the MU2 models at four wavelengths, from left to right: 24 μm, 70 μm, 160 μm, and 1200 μm. Three different times are shown that trace the evolutionary stage of the source: t0 − 26.43 kyr (top row, i.e., starless core), t0 + 0.7 kyr (middle row, i.e., faint FHSC) and t0 + 1.13 kyr (bottom row, i.e., end of the FHSC lifetime). The fluxes are given in Jy/px (1 px = 0.08′′ × 0.08′′) for objects at a distance of 150 pc and observed pole-on.

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