Document Type
Article
Publication Date
12-16-2024
Abstract
2-Cyanoindene is one of the few specific aromatic or polycyclic aromatic hydrocarbon (PAH) molecules positively identified in Taurus molecular cloud-1 (TMC-1), a cold, dense molecular cloud that is considered the nearest star-forming region to Earth. We report cryogenic mid-infrared (550–3200 cm–1) and visible (16,500–20,000 cm–1, over the D2 ← D0 electronic transition) spectra of 2-cyanoindene radical cations (2CNI+), measured using messenger tagging (He and Ne) photodissociation spectroscopy. The infrared spectra reveal the prominence of anharmonic couplings, particularly over the fingerprint region. There is a strong CN-stretching mode at 2177 ± 1 cm–1 (4.593 μm), which may contribute to a broad plateau of CN-stretching modes across astronomical aromatic infrared band spectra. However, the activity of this mode is suppressed in the dehydrogenated (closed shell) cation, [2CNI-H]+. The IR spectral frequencies are modeled by anharmonic calculations at the B3LYP/N07D level of theory that include resonance polyad matrices, demonstrating that the CN-stretch mode remains challenging to describe with theory. The D2 ← D0 electronic transition of 2CNI+, which is origin dominated, occurs at 16,549 ± 5 cm–1 in vacuum (6041.8 Å in air). There are no correspondences with reported diffuse interstellar bands.
Recommended Citation
Douglas-Walker T., Ashworth E. K., Stockett M. H., Daly F., Chambrier I., Esposito V. J., Gerlach M., Cammidge A. N., Campbell E. K., Brünken S., Bull J. N. “Vibrational and Electronic Spectroscopy of 2-Cyanoindene Cations.” ACS Earth Space Chem. 9, 134 (2025). https://doi.org/10.1021/acsearthspacechem.4c00270
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Comments
This article was originally published in ACS Earth and Space Chemistry, volume 9, issue 1, in 2025. https://doi.org/10.1021/acsearthspacechem.4c00270