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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- Early Science from GOTHAM: Project Overview, Methods, and the Detection of Interstellar Propargyl Cyanide (HCCCHCN) in TMC-1
- Discovery of HC4NC in TMC-1: A study of the isomers of HC3N, HC5N, and HC7N
- Discovery of the acetyl cation, CH3CO+, in space and in the laboratory
- Astronomical Detection of the Interstellar Anion C10H- towards TMC-1 from the GOTHAM Large Program on the GBT
- Machine Learning of Interstellar Chemical Inventories
- Detection of Interstellar -1-cyano-1,3-butadiene in GOTHAM Observations of TMC-1
- Discovery of Interstellar trans-cyanovinylacetylene (HCCCH=CHCN) and vinylcyanoacetylene (HC=CHCN) in GOTHAM Observations of TMC-1
- Chemical variations across the TMC-1 boundary: molecular tracers from translucent phase to dense phase