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Fig. 9.
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Dust opacity τ100 μm vs. SFR surface density ΣSFR. The dashed line shows a fit to the data points under the optically thin assumption, i.e., τ100 μm = 3.1 × 10−2ΣSFR. In both the optically thin and thick models, our sample shows high dust opacity at FIR wavelengths.
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