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Fig. A.1.


Spectral energy distribution based on Herschel (Molinari et al. 2016) and LABOCA data (Schuller et al. 2009) for G10.99−0.08 (top panel) and G28.33+0.07 (bottom panel). The data at different wavelengths are shown as squares with error bars. The temperature and bolometric luminosity obtained based on the SED fit assuming a dust opacity (β = 1.8) is also shown (König et al. 2017).

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