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Fig. 7

image

Relative abundances of HCO+, HNC, and C2H observed in absorption with respect to H2 plotted against the local spaced-averaged mean H2 density derived from CH (at left) and galactocentric radius (at right). Column and number densities of H2 were derived from the CH absorption profile as discussed in Sect. 4 of the text. The mean relative abundances ± 1σ and power-law slopes of the fitted regression lines are shown in the individual panels.

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