Fig. 8
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Integrated emission maps from the Mopra survey, showing the three detected molecular structures, identified with capital letters. Top panel: CO emission distribution. White contour values of 8.6 and 9.9 Κ are drawn. Bottom panel: 13CO emission distribution. The white contours correspond to 2 and 2.8 K. Both maps have been integrated along the line of sight, in the velocity interval from −98 km s−1 to −86 km s−1. The blue asterisk indicates the position of the WR star, and the yellow one, the position of the O-type star.
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