Fig. 1
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Comparison between the flux recovered towards OMC-2 FIR4 by single-dish IRAM 30 m observations (red) and towards the region equivalent to the 30 m primary beam within the interferometric IRAM NOEMA observations of the same source (black). The figure shows that we recover approximately 20% of the flux in both the H13CN line and the HC15N lines. The line at 86.1GHz is SO (22−11).
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