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Fig. 4
Far-infrared and submillimeter continuum fluxes of MSXG52 in the Herschel 160, 250, 350 and 500 μm bands. The red line is the best-fit graybody model (Eq. (6)) corresponding to a dust temperature of ~48 K and H2 column density of ~ 2 × 1021 cm-2.
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