Reproduction of Interstellar Infrared Spectrum of Reflection Nebula NGC2023 By A Hydrocarbon Pentagon-Hexagon Combined Molecule
Norio Ota

TL;DR
This study demonstrates that ionized hydrocarbon molecules with pentagon-hexagon structures can accurately reproduce the infrared spectrum observed in the reflection nebula NGC2023, providing insights into interstellar PAH carriers.
Contribution
The paper introduces specific hydrocarbon pentagon-hexagon combined molecules as carriers for interstellar infrared spectra, validated by detailed spectral comparison.
Findings
Successful reproduction of observed IR bands by model molecules
Hydrocarbon pentagon-hexagon structures match interstellar spectra
Single molecule models can explain complex IR features
Abstract
Reflection Nebula NGC2023 shows specific interstellar infrared spectrum due to polycyclic aromatic hydrocarbon (PAH) in a wide wavelength range from 5 to 20 micrometer. By our previous quantum chemistry calculation, it was suggested that a molecule group having hydrocarbon pentagon-hexagon combined skeleton could reproduce ubiquitous interstellar infrared spectrum. In this paper, observed NGC2023 spectrum was compared in detail with such carrier candidates. First model molecule was di-cation (C23H12)2+ with two hydrocarbon pentagons combined with five hexagons. Observed strong infrared bands were 6.2, 7.7, 8.6, and 11.2 micrometer. Whereas, calculated strong peaks were 6.4, 7.5, 7.7, 8.5, and 11.2 micrometer. Observed weaker bands from 10 to 15 micrometer were 11.0, 12.0, 12.7, 13.5, and 14.2 micrometer, which were reproduced well by computed bands as 10.9, 12.0, 12.6, 13.6, and 14.0…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsPhotochemistry and Electron Transfer Studies · Atmospheric Ozone and Climate · Astrophysics and Star Formation Studies
