Polycyclic Aromatic Hydrocarbons with armchair edges and the 12.7 μm band
arXiv:1407.2010 · doi:10.1088/2041-8205/791/1/L10
Abstract
In this Letter we report the results of density functional theory calculations on medium-sized neutral Polycyclic Aromatic Hydrocarbon (PAH) molecules with armchair edges. These PAH molecules possess strong C-H stretching and bending modes around 3 μm and in the fingerprint region (10-15 μm), and also strong ring deformation modes around 12.7 μm. Perusal of the entries in the NASA Ames PAHs Database shows that ring deformation modes of PAHs are common - although generally weak. We then propose that armchair PAHs with NC >65 are responsible for the 12.7 μm Aromatic Infrared Band in HII regions and discuss astrophysical implications in the context of the PAH life-cycle.
Minor editing
References in corpus (1)
Cited by in corpus (10)
- Laboratory formation of fullerenes from PAHs: Top-down interstellar chemistry
- The PAH emission characteristics of the reflection nebula NGC2023
- The 11.2 m emission of PAHs in astrophysical objects
- Investigating the importance of edge-structure in the loss of H/H2 of PAH cations: the case of dibenzopyrene isomers
- On the Origin of the 3.3 Micron Unidentified Infrared Emission Feature
- Mechanochemical synthesis of Aromatic Infrared Band carriers. The top-down chemistry of interstellar carbonaceous dust grain analogues
- Interstellar dehydrogenated PAH anions: vibrational spectra
- Machine-learning identified molecular fragments responsible for infrared emission features of polycyclic aromatic hydrocarbons
- A Principal Component Analysis of polycyclic aromatic hydrocarbon emission in NGC 7023
- IRMPD spectroscopy of a PAH cation using FELICE: The infrared spectrum and photodissociation of dibenzo[a,l]pyrene