Work supported by the Department of Energy (Office of Basic Energy Science)Author Institution: National Institute for Petroleum and Energy ResearchThe region from 2000 to $1650 cm^{-1}$ in the infrared vapor spectrum for indole and related compounds exhibits several transitions, none of which are due to fundamentals. Careful analysis shows that nearly all of these should be assigned to overtones/combinations of the out-of-plane wags of the hydrogen groups. In a few cases, the fundamental itself is not observable in the infrared vapor spectrum due to low transition strength. The results help to pinpoint the location of these particular fundamentals and give an indication of the amount of anharmonicity as well. The complete set of wag frequen...
ISO has shown that the mid-IR spectra, of almost all sources are dominated by narrow emission featur...
Author Institution: McLennan Laboratory, University of Toronto“Previous work has shown that the fund...
ISO has shown that the mid-IR spectra of almost all sources are dominated by narrow emission feature...
Author Institution: Physical Chemistry, Eth ZUrich, Ch-8093 ZUrich, Switzerland; SWISS LIGHT SOURCE,...
Context. The 3.3 μm aromatic C–H stretching band of polycyclic aromatic hydrocarbon (PAH) molecules ...
Aims. Infrared (IR) spectroscopy is a powerful tool to study molecules in space. A key issue in such...
Author Institution: Department of Chemistry, The Ohio State University, Columbus, OH 43210As the inf...
Author Institution: University of Waterloo, Waterloo, Ontario, N2L 3G1Recording the spectra of gas-p...
Although large polycyclic aromatic hydrocarbons (PAHs) are likely to be responsible for IR emission ...
The unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, 11.3 and 12.7 µm are ubiqu...
Unidentified InfraRed emission bands (uirs) have intrigued astronomers ever since their discovery in...
The profile of the 11.2 μm feature of the infrared (IR) cascade emission spectra of polycyclic aroma...
The infrared (IR) emission of polycyclic aromatic hydrocarbons (PAHs) permeates our universe; astron...
Gas-phase infrared (IR) spectra of larger protonated polycyclic aromatic hydrocarbon molecules, H(+)...
ISO has shown that the mid-IR spectra, of almost all sources are dominated by narrow emission featur...
Author Institution: McLennan Laboratory, University of Toronto“Previous work has shown that the fund...
ISO has shown that the mid-IR spectra of almost all sources are dominated by narrow emission feature...
Author Institution: Physical Chemistry, Eth ZUrich, Ch-8093 ZUrich, Switzerland; SWISS LIGHT SOURCE,...
Context. The 3.3 μm aromatic C–H stretching band of polycyclic aromatic hydrocarbon (PAH) molecules ...
Aims. Infrared (IR) spectroscopy is a powerful tool to study molecules in space. A key issue in such...
Author Institution: Department of Chemistry, The Ohio State University, Columbus, OH 43210As the inf...
Author Institution: University of Waterloo, Waterloo, Ontario, N2L 3G1Recording the spectra of gas-p...
Although large polycyclic aromatic hydrocarbons (PAHs) are likely to be responsible for IR emission ...
The unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, 11.3 and 12.7 µm are ubiqu...
Unidentified InfraRed emission bands (uirs) have intrigued astronomers ever since their discovery in...
The profile of the 11.2 μm feature of the infrared (IR) cascade emission spectra of polycyclic aroma...
The infrared (IR) emission of polycyclic aromatic hydrocarbons (PAHs) permeates our universe; astron...
Gas-phase infrared (IR) spectra of larger protonated polycyclic aromatic hydrocarbon molecules, H(+)...
ISO has shown that the mid-IR spectra, of almost all sources are dominated by narrow emission featur...
Author Institution: McLennan Laboratory, University of Toronto“Previous work has shown that the fund...
ISO has shown that the mid-IR spectra of almost all sources are dominated by narrow emission feature...