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Fig. 9


Comparison of the ISM gas components as a function of Galactocentric radius RG. The spaxels for RG<R (8.5 kpc) are the only ones used (see Table 2) for the analysis. a) Histogram representation of the number distribution of spaxels detected in H i, [C ii], and 12CO as a function RG (upper panel). Number of detections of the [C ii] and CO components (lower panel). b) Detection rates of [C ii] (upper panel) and CO (lower panel) components (normalized using the number of H i spaxels in each RG-bin as measure of the sampled volume) as function RG.

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