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Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features
The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lyi...
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Published in: | The Astrophysical journal 1996-12, Vol.472 (2), p.L127-L130 |
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container_end_page | L130 |
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container_title | The Astrophysical journal |
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creator | Bernstein, Max P Sandford, Scott A Allamandola, Louis J |
description | The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lying fundamentals. The aliphatic C-H stretches in molecules of this type having low to modest excess H coverage provide excellent fits to a number of the weak emission features superposed on the plateau between 3080 and 2700 cm-1 (3.25 and 3.7 microns) in the spectra of many planetary nebulae, reflection nebulae, and H II regions. Higher H coverage is implied for a few objects. We compare these results in context with the other suggested identifications of the emission features in the 2950-2700 cm-1 (3.39-3.70 microns) region and briefly discuss their astrophysical implications. |
doi_str_mv | 10.1086/310376 |
format | article |
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source | EZB Electronic Journals Library |
subjects | Astronomy - methods Extraterrestrial Environment Hydrocarbons, Alicyclic - chemistry Hydrogen - chemistry Polycyclic Aromatic Hydrocarbons - analysis Polycyclic Aromatic Hydrocarbons - chemistry Space life sciences Spectrophotometry, Infrared |
title | Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features |
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