Testing analytical methods to derive the cosmic-ray ionisation rate in cold regions via synthetic observations

Open Access

Fig. B.1

Ratio between the sum of the rates of the reactions between ${pH}_{3}^{+}$ ${\rm{pH}}_3^ +$ and HD and those involving ${oH}_{3}^{+}$ ${\rm{oH}}_3^ +$ and HD, as a function of temperature. Right panel: the ratio between the total rate of dissociative recombination of ${pH}_{3}^{+}$ ${\rm{pH}}_3^ +$ and that of ${oH}_{3}^{+}$ ${\rm{oH}}_3^ +$ , as a function of temperature. In both panels, the horizontal dashed lines correspond to unity.

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