CH3-Terminated Carbon Chains in the GOTHAM Survey of TMC-1: Evidence of Interstellar CH3C7N
arXiv:2110.13152 · doi:10.3847/1538-4357/ac3238
Abstract
We report a systematic study of all known methyl carbon chains toward TMC-1 using the second data release of the GOTHAM survey, as well as a search for larger species. Using Markov-Chain Monte Carlo simulations and spectral line stacking of over 30 rotational transitions, we report statistically significant emission from methylcyanotriacetylene (CHCN) at a confidence level of 4.6, and use it to derive a column density of 10 cm. We also searched for the related species, methyltetraacetylene (CHCH), and place upper limits on the column density of this molecule. By carrying out the above statistical analyses for all other previously detected methyl-terminated carbon chains that have emission lines in our survey, we assess the abundances, excitation conditions, and formation chemistry of methylpolyynes (CH3CH) and methylcyanopolyynes (CH3CN) in TMC-1, and compare those with predictions from a chemical model. Based on our observed trends in column density and relative populations of the A and E nuclear spin isomers, we find that the methylpolyynes and methylcyanopolyynes families exhibit stark differences from one another, pointing to separate interstellar formation pathways, which is confirmed through gas-grain chemical modeling with nautilus.
15 pages, 7 figures. Accepted for publication in ApJ
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Cited by in corpus (8)
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- Carbon-Chain Chemistry in the Interstellar Medium
- Astronomical Detection of the Interstellar Anion C10H- towards TMC-1 from the GOTHAM Large Program on the GBT
- Astrochemical Modeling of Propargyl Radical Chemistry in TMC-1
- Millimetre and submillimetre spectroscopy of isobutene and its detection in the molecular cloud G+0.693
- A search for the three isomers of cyano-1,3-butadiene in TMC-1: Implications for bottom-up routes involving 1,3-butadiene
- Carbon chain diversity in L1544 and IRAS 16293-2422: an astrochemical pathfinder study for the SKAO