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Fig. 5


Physical-chemical model of IRS 48 from Bruderer et al. (2014). The panels show gas density (cm-3), gas temperature (K), CO abundance with respect to H2, dust density (cm-3), dust temperature (K), and UV field in G0 (G0 = 1 refers to the standard interstellar radiation field). The given numbers are in 10log scale.

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