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Fig. 8


Comparison of the gas components of [C ii] emission as a function of H i intensity for Galactocentric radius RG<R (8.5 kpc); and for different values of b as indicated in panels a) to e) (see Table 2). a) The fraction of detections of [C ii] and 12CO components and combinations of [C ii] and CO (as indicated by the colors) plotted against H i intensity. b) Histogram representation of the number distribution of spaxels detected in H i, [C ii], and 12CO as a function of H i intensity. c)e) The number of [C ii] detections compared with the H i intensity shown for each absolute value of the latitude separately. The [C ii] detections with and without CO are plotted separately to bring out differences between the dense and diffuse components of [C ii] emission.

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