The C--H Stretching Features at 3.2--3.5 Micrometer of Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups
Xuejuan Yang, Aigen Li, Rainer Glaser, Jianxin Zhong

TL;DR
This study uses density functional theory to analyze the infrared vibrational spectra of PAHs with various sidegroups, improving understanding of the aliphatic fraction in UIE carriers and confirming their predominantly aromatic nature.
Contribution
It provides new computational data on PAHs with diverse sidegroups, refining estimates of aliphatic content in UIE carriers beyond previous mono-methyl studies.
Findings
A3.4/A3.3 ratios are similar to mono-methyl PAHs for most sidegroups
Confirms UIE carriers are predominantly aromatic
Provides theoretical oscillator strengths for diverse PAHs
Abstract
The so-called unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 micrometer are ubiquitously seen in a wide variety of astrophysical regions. The UIE features are characteristic of the stretching and bending vibrations of aromatic hydrocarbon materials, e.g., polycyclic aromatic hydrocarbon (PAH) molecules. The 3.3 micrometer aromatic C--H stretching feature is often accompanied by a weaker feature at 3.4 micrometer. The latter is often thought to result from the C--H stretch of aliphatic groups attached to the aromatic systems. The ratio of the observed intensity of the 3.3 micrometer aromatic C--H feature to that of the 3.4 micrometer aliphatic C--H feature allows one to estimate the aliphatic fraction of the UIE carriers, provided that the intrinsic oscillator strengths of the 3.3 micrometer aromatic C--H stretch (A3.3) and the 3.4 micrometer aliphatic C--H…
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