Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...388l..39b&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 388, March 20, 1992, p. L39-L43. Research supported by NSF and DO
Astronomy and Astrophysics
Astrophysics
53
Benzene, Emission Spectra, Infrared Spectra, Interstellar Matter, Naphthalene, Astronomical Spectroscopy, Electron Transitions, Molecular Excitation, Vibrational Spectra
Scientific paper
Results are presented of observations of emissions from the fundamental region (about 3050/cm, 3.3 microns) and first overtone (about 6000/cm, 1.7 micron) of the C-H stretching modes in C6H6 and C10H8 which were performed following UV laser excitations. Wavelength- and time-resolved emission spectra in the 3050/cm region show contributions from anharmonically shifted Delta-v = -1 transitions originating in v = 1, 2, and 3 in C6H6 and v = 1 and 2 in C10H8, as well as underlying continuum emission. The measured anharmonicities agree with literature values, and relative intensities match those predicted by theory for Delta-v = -1 transitions. The emission transition frequencies differ significantly from the corresponding absorption frequencies for both molecules, and depend on the vibrational energy of the emitter. It is concluded that unambiguous identification of the interstellar emitters cannot be established just on the basis of matching the emission frequencies to laboratory absorption spectra.
Barker John R.
Brenner Jerrell
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