Fig. 2
ALMA observations of CO(3–2) towards the Mira AB system at vlsr = 43.3 km s−1. The white and blue plus symbols show the positions of omi Cet (Mira A) and VZ Cet (Mira B), respectively. The contours are overlaid on the image with 20, 35, and 50% of the peak value. The observed CI emission likely arises from the region near Mira B. The beam is shown in the lower left corner.
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