Fig. 22
Comparison between the [C ii] and 12CO emissivities corresponding to different Galactocentric rings, for gas associated with Mask 3 (red circles) and Mask 4 (black boxes). The straight lines represent fits to the data. Typical uncertainties are 0.02 and 0.1 K km s-1 kpc-1, for [C ii] and 12CO, respectively.
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