The interstellar gas-phase chemistry of HCN and HNC

• Published in: Monthly notices of the Royal Astronomical Society 2014-09, Vol.443 (1), p.398-410
• Main Authors: Loison, Jean-Christophe, Wakelam, Valentine, Hickson, Kevin M.
• Format: Article
• Language: English
• Subjects: Astronomical research; Astrophysics; Chemical reactions; Clouds; Cosmology and Extra-Galactic Astrophysics; Hydrogen; Physics; Sciences of the Universe
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stu1089

We review the reactions involving hydrogen cyanide (HCN) and hydrogen isocyanide (HNC) in dark molecular clouds to elucidate new chemical sources and sinks of these isomers. We find that the most important reactions for the HCN–HNC system are dissociative recombination (DR) reactions of HCNH+ (HCNH+ + e−), the ionic CN + H3 +, HCN + C+, HCN and HNC reactions with H+/He+/H3 +/H3O+/HCO+, the N + CH2 reaction and two new reactions: H + CCN and C + HNC. We test the effect of the new rate constants and branching ratios on the predictions of gas–grain chemical models for dark cloud conditions. The rapid C + HNC reaction keeps the HCN/HNC ratio significantly above 1 as long as the carbon atom abundance remains high. However, the reaction of HCN with H3 + followed by DR of HCNH+ acts to isomerize HCN into HNC when carbon atoms and CO are depleted leading to an HCN/HNC ratio close to or slightly greater than 1. This agrees well with observations in TMC-1 and L134N taking into consideration the overestimation of HNC abundances through the use of the same rotational excitation rate constants for HNC as for HCN in many radiative transfer models.