Fig. 4
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Integrated intensity maps at 1.4 mm observed with the IRAM 30m telescope towards the G183 region. The colour plot in each panel is the integrated emission of C18O(2–1) and the contours correspond to molecular transitions, as is indicated above the panels. The intensities are integrated between velocities of −20 to 0 km s−1. The HPBW is shown on the lower right.
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