Fig. 6.

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3.2 × IHCN/ICO as a function of the fraction of gas above (from left to right) n ∼ 102.5, 103.5, 104.5, and 105.5 cm−3. The formatting is the same as in Fig. 3. The fits are shown as the solid black line (see legend). The modeled IHCN/ICO scales most directly (has a slope closest to unity) with f(n > 103.5 cm−3), supporting previous findings that this line ratio is sensitive to gas above moderate densities. Although not shown here, the same is found when comparing the emissivity ratio, ⟨ϵHCN⟩/⟨ϵCO⟩, with the same gas fractions. The Spearman rank coefficients are shown in the lower right corner of each plot.
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