Fig. 2

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Maps of the DCO+ and H13CO+ (1−0) emission obtained with NOEMA and 30 m telescopes. The beam size and scale bar are shown in the top left and bottom right, respectively. The contours correspond to the Herschel-based H2 column map; the first level is at log10(N(H2)) = 22.2, and the step between levels is 0.5 dex. The stars mark the positions of the YSOs identified by Dunham et al. (2015) using Spitɀer observations.
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