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Fig. 4

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Integrated emission line brightnesses for HCO+J = 1−0 (red boxes), CS J = 2−1 (green diamonds) and HCN J = 1−0 (magenta parallelogram) observed in diffuse gas, plotted against the integrated brightness of CO J = 1−0. Data sources are given in Sects. 4.1–4.3. Chained red and green curves are model results as discussed in Sect. 4.4. For both HCO+ (red) and CS (green), calculations are shown for clouds with N(H) = 0.7 and 2.0  × 1021  cm-2 with number density n(H) increasing from 128  cm-3 at left in marked steps of 21/2. X(HCO+) = X(CS)  = 2 × 10-9 was assumed; the CS brightness increases linearly with increased abundance X(CS) at fixed WCO while that of HCO+ declines very slightly, as discussed in Sect. 4.4 of the text.

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