First detection in space of the high-energy isomer of cyanomethanimine: H2CNCN
arXiv:2404.03334 · doi:10.3847/1538-4357/ad3af3
Abstract
We report the first detection in the interstellar medium of -cyanomethanimine (HCNCN), the stable dimer of HCN of highest energy, and the most complex organic molecule identified in space containing the prebiotically relevant NCN backbone. We have identified a plethora of -type rotational transitions with 3 11 and 2 that belong to this species towards the Galactic Center G+0.693-0.027 molecular cloud, the only interstellar source showing the three cyanomethanimine isomers (including the - and - isomers of -cyanomethanimine, HNCHCN). We have derived a total column density for HCNCN of (2.90.1)10 cm, which translates into a total molecular abundance with respect to H of (2.10.3)10. We have also revisited the previous detection of - and -HNCHCN, and found a total -cyanomethanimine abundance ratio of 31.81.8 and a -HNCHCN ratio of 4.50.2. While the latter can be explained on the basis of thermodynamic equilibrium, chemical kinetics are more likely responsible for the observed -cyanomethanimine abundance ratio, where the gas-phase reaction between methanimine (CHNH) and the cyanogen radical (CN) arises as the primary formation route.
22 pages, 8 figures, 3 tables, 2 appendix - Accepted for publication in The Astrophysical Journal
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