Published October 20, 2013 | Version v1
Journal article

THE INFRARED SPECTRA OF POLYCYCLIC AROMATIC HYDROCARBONS WITH SOME OR ALL HYDROGEN ATOMS REMOVED

  • 1. Entry Systems and Technology Division, Mail Stop 230-3, NASA Ames Research Center, Moffett Field, CA 94035 (United States)
  • 2. Carl Sagan Center, SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043 (United States)

Description

The loss of one hydrogen from C96H24 does not significantly affect the infrared spectra of the neutral, cation, or anion. Excluding a very weak C-C stretching band at 5.1 μm, the loss of two adjacent duo hydrogens does not significantly affect the spectra compared with the parent. Removing all of the hydrogen atoms significantly increases the intensity of the new C-C stretching band, and, for the cation, shifts it to a longer (5.2 μm) wavelength. Observations show a feature near 5.25 μm, which has been attributed to overtone and combination bands from polycyclic aromatic hydrocarbons (PAHs). This current work suggests that dehydrogenated PAHs might also contribute to this band, but its weakness implies that fully dehydrogenated cationic or dicationic species are very rare

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/776/2/102

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
776
Journal Issue
2
Journal Page Range
[9 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
45092019
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ASTRONOMY; ASTROPHYSICS; ATOMS; COMPARATIVE EVALUATIONS; COSMOCHEMISTRY; HYDROGEN; INFRARED SPECTRA; MOLECULES; POLYCYCLIC AROMATIC HYDROCARBONS; WAVELENGTHS
Descriptors DEC
AROMATICS; CHEMISTRY; ELEMENTS; EVALUATION; HYDROCARBONS; NONMETALS; ORGANIC COMPOUNDS; PHYSICS; SPECTRA