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. Author manuscript; available in PMC: 2017 Nov 13.
Published in final edited form as: Astron Astrophys. 2017 Sep 21;605:A126. doi: 10.1051/0004-6361/201730934

Fig. 2.

Fig. 2

Comparison between the direction-averaged CO(J = 3→2) brightness distribution from the ALMA observations (red dots with error bars) and that derived from the radiative transfer model assuming a spherically symmetric CSE (blue dots).