Fig. 2
Observed spectral energy distribution (SED) of Serpens SMM1 and modified blackbody fit (red curve). Inset shows the full PACS array in flux density units of 10-14 W m-2 μm-1. The abscissa is in linear scale from 55 to 190 μm. The bright emission line seen in several positions is [O i]63 μm. Approximate outflow directions are shown with red and blue arrows.
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