Fig. 16

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Radial distribution of the azimuthally averaged 12CO and 13CO emissivities observed in the Galactic plane for the case where 12CO is detected in individual spaxels but 13CO is not (mask CO1; upper panel), and for the case where both 12CO and 13CO are detected in individual spaxels (mask CO2; lower panel). Typical uncertainties of the 12CO and 13CO emissivities are 0.1 and 0.02 K km s-1 kpc-1, respectively.

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