Fig. 21

Top panel: radial distribution of the surface density of hydrogen in the Galactic plane. We also show the contribution of the atomic and molecular hydrogen gas. Lower panel: radial distribution of the different ISM components, including the cold and warm neutral medium (atomic gas), the CO-dark H2 component, and the H2 gas that is traced by 12CO and 13CO. All surface densities have been corrected to account for the contribution of He.
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