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Fig. 2.

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Spectral energy distribution of D49. The red open squares and downward arrow indicate the fitted photometry and upper limits. The black line shows the Stardust best-fit SED, while the contribution from stars and dust are respectively shown as a blue and red filled region. The grey region presents the predicted contribution from radio continuum, based on the radio-FIR model described in Delvecchio et al. (2021).

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