Fig. 7
Following Fig. 6. Bottom left panel: black contours show the JCMT/SCUBA-2/450 μm emission presented in Tigé et al. (2017). The contours range from 20 to 90% of the peak flux inside the MDC #26 (defined by the blue ellipse) by step of 10%. They show that the continuum source ALMA#38 is associated with the MDC #26, while the continuum sources ALMA#3, #4, and #35 belong to another structure.
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