2016ApJ...825...22Y

The so-called "unidentified" infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 µm 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 µm aromatic C-H stretching feature is often accompanied by a weaker feature at 3.4 µm. The latter is generally 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 µm aromatic C-H feature to that of the 3.4 µm 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 µm aromatic C-H stretch ( {A}_{3.3} ) and the 3.4 µm aliphatic C-H stretch ( {A}_{3.4} ) are known. While previous studies on the aliphatic fraction of the UIE carriers were mostly based on the {A}_{3.4}/{A}{3.3} ratios derived from the mono-methyl derivatives of small PAH molecules, in this work we employ density functional theory to compute the infrared vibrational spectra of PAH molecules with a wide range of sidegroups including ethyl, propyl, butyl, and several unsaturated alkyl chains, as well as all the isomers of dimethyl-substituted pyrene. We find that, except for PAHs with unsaturated alkyl chains, the corresponding {A}_{3.4}/{A}{3.3} ratios are close to that of mono-methyl PAHs. This confirms the predominantly aromatic nature of the UIE carriers previously inferred from the {A}_{3.4}/{A}{3.3} ratio derived from mono-methyl PAHs.