Left: dust extinction map of the Chamaeleon-Musca region, based on 2MASS data (Kainulainen et al. 2009). Right: zoom-in to the Musca cloud, showing the instrument footprints of the observations employed in this work: NEWFIRM/NIR data (red rectangles), LABOCA/870 μm continuum emission (blue dashed lines, approximate coverage), SHeFI/C18O line emission (green crosses, from Hacar et al. 2016).
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