Fig. A.1

Total intensity of the 12CO and 13CO(J = 3 → 2) transitions. The solid black lines are the spectra observed with the APEX telescope in a single pointing towards the star. The solid red line is the emission detected with ALMA in an area equivalent to the APEX beam. The 13CO ALMA spectrum has a velocity resolution of 3 km s-1, the 12CO ALMA spectrum has a velocity resolution of 0.5 km s-1, and the APEX spectra have a velocity resolution of 1.1 km s-1. The dotted line indicates the 13CO model used to fit the ALMA observations (see text) when observed with APEX resolution. The spectra indicate that the 12CO and 13CO emissions are equally resolved out in the ALMA observations.
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