Discovery of Interstellar 2-Cyanoindene (2-CHCN) in GOTHAM Observations of TMC-1
arXiv:2209.06851 · doi:10.3847/2041-8213/ac92f4
Abstract
We present laboratory rotational spectroscopy of five isomers of cyanoindene (2-, 4-, 5-, 6-, and 7-cyanoindene) using a cavity Fourier-transform microwave spectrometer operating between 6-40 GHz. Based on these measurements, we report the detection of 2-cyanoindene (1H-indene-2-carbonitrile; 2-CHCN) in GOTHAM line survey observations of the dark molecular cloud TMC-1 using the Green Bank Telescope at centimeter wavelengths. Using a combination of Markov Chain Monte Carlo (MCMC), spectral stacking, and matched filtering techniques, we find evidence for the presence of this molecule at the 6.3 level. This provides the first direct observation of the ratio of a cyano-substituted polycyclic aromatic hydrocarbon (PAH) to its pure hydrocarbon counterpart, in this case indene, in the same source. We discuss the possible formation chemistry of this species, including why we have only detected one of the isomers in TMC-1. We then examine the overall hydrocarbon:CN-substituted ratio across this and other simpler species, as well as compare to those ratios predicted by astrochemical models. We conclude that while astrochemical models are not yet sufficiently accurate to reproduce absolute abundances of these species, they do a good job at predicting the ratios of hydrocarbon:CN-substituted species, further solidifying -CN tagged species as excellent proxies for their fully-symmetric counterparts.
Accepted in ApJL
References in corpus (9)
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- Aromatic cycles are widespread in cold clouds
- Detection of Interstellar -1-cyano-1,3-butadiene in GOTHAM Observations of TMC-1
- Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey
- Low NH/HO ratio in comet C/2020 F3 (NEOWISE) at 0.7 au from the Sun
- CN and CCH derivatives of ethylene and ethane: Confirmation of the detection of CHCHCCH in TMC-1
- On the spectroscopy of phosphaalkynes: Millimeter- and submillimeter wave study of C2H5CP
- Concluding remarks: Faraday Discussion on astrochemistry at high resolution