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. Author manuscript; available in PMC: 2017 Nov 15.
Published in final edited form as: Astron Astrophys. 2017 Nov 9;607:L5. doi: 10.1051/0004-6361/201732015

Fig. 1.

Fig. 1

Comparison of the central channel of the low spatial resolution 3mm stacked map with maps of the ALMA Cycle 4 observations at 2 mm. The lowest contour corresponds to 10% of the peak flux, and the rest of contours are equally spaced in jumps of 10% with respect to the first contour. For absolute intensities see Figs.A.1,A.4, and A.5.