Ion鈥搈olecule reactions are thought to play a crucial role in the formation of metastable isomers, but relatively few protonated intermediates beyond HNCH
+ have been characterized at high spectral resolution. We present here laboratory measurements of the rotational spectra of protonated isocyanic acid in two isomeric forms, the ground state H
2NCO
+ with
C2v symmetry and a low-lying bent chain HNCOH
+, guided by coupled cluster calculations of their molecular structure. Somewhat surprisingly, HNCOH
+ is found to be more abundant than H
2NCO
+, even though this metastable isomer is calculated to lie approximately 15鈥?0 kcal/mol higher in energy. In the same way that HCNH
+ serves as a key intermediate in ion鈥搈olecule reactions that form HNC via dissociative electron recombination in cold dense interstellar molecular clouds, HNCOH
+ may play an analogous role in the conversion of HNCO to HOCN.
Keywords:
rotational spectroscopy; quantum-chemical calculations; astronomy&qsSearchArea=searchText">radio astronomy; molecular structure; bonding