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Fig. 3

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Equatorial ring model (white) of the 12CO and 13CO emission of NGC 6778 overlaid on an image of the nebula taken with the NOT telescope (adapted from Guerrero & Miranda 2012). White crosses mark the observed offset positions, while associated insets show their corresponding 12CO J = 2–1 emission profiles (black) and SHAPE+SHAPEMOL model synthetic profiles (red). The HPBW of the IRAM 30m telescope at the 12CO J = 2–1 transition is indicated by the white circle.

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