Infrared Emission of Specific Polycyclic Aromatic Hydrocarbon Molecules: Cyanonaphthalenes

The unidentified infrared emission features at 3.3, 6.2, 7.7, 8.6, 11.3, and 12.7 μ m are ubiquitously seen in a wide variety of astrophysical regions and commonly attributed to polycyclic aromatic hydrocarbon (PAH) molecules. However, the unambiguous identification of any individual, specific PAH m...

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Hlavní autoři:	Kaijun Li, Aigen Li, X. J. Yang, Taotao Fang
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astrophysical Journal
Témata:	Polycyclic aromatic hydrocarbons Infrared spectroscopy Interstellar emissions Interstellar molecules
On-line přístup:	https://doi.org/10.3847/1538-4357/ad1508
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