paper

Detection of Interstellar HCNC and an Investigation of Isocyanopolyyne Chemistry under TMC-1 Conditions

arXiv:2008.12345 · doi:10.3847/2041-8213/aba631

Abstract

We report an astronomical detection of HCNC for the first time in the interstellar medium with the Green Bank Telescope toward the TMC-1 molecular cloud with a minimum significance of . The total column density and excitation temperature of HCNC are determined to be cm and K, respectively, using the MCMC analysis. In addition to HCNC, HCCNC is distinctly detected whereas no clear detection of HCNC is made. We propose that the dissociative recombination of the protonated cyanopolyyne, HCNH, and the protonated isocyanopolyyne, HCNCH, are the main formation mechanisms for HCNC while its destruction is dominated by reactions with simple ions and atomic carbon. With the proposed chemical networks, the observed abundances of HCNC and HCCNC are reproduced satisfactorily.

Accepted in the Astrophysical Journal Letters

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