Fig. 3.

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Low resolution channel map of 12CO v = 0 J = 2 − 1 in IRC −10529. The peak of the continuum emission is at (0,0). The velocity (in km s−1) is with respect to the stellar velocity of −16.3 km s−1 (see the last column in Table 1), and is indicated in the upper right corner of each panel. The ALMA synthesized beam is shown as a white ellipse in the lower left corner of each panel (see Table E.2). The offsets in right ascension and declination are with respect to the peak of the continuum emission.
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