Infrared bands of the C2 Phillips system

Details Infrared bands of the C2 Phillips system Infrared bands of the C2 Phillips system

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988josab...5.2280d&link_type=abstract

Optical Society of America, Journal, B: Optical Physics (ISSN 0740-3224), vol. 5, Oct. 1988, p. 2280-2285. NSF-supported researc

Physics

14

Carbon, Carbon Stars, Comet Tails, Infrared Spectra, Stellar Atmospheres, Vibrational Spectra, Fourier Transformation, Line Spectra, Spectrum Analysis

Scientific paper

The spectrum of the C2 Phillips system was observed in the spectral region 3300-6500/cm by using a high-resolution Fourier-transform spectrometer and a hollow-cathode discharge source. Three new bands were observed, the (2-3), (1-3), and (2-4) bands belonging to the Delta v = -1 and Delta v = -2 sequences. In addition, new lines were observed in the (0-2) band. These lines, combined with previous high-resolution data, are used in a linear least-squares algorithm to calculate Dunham coefficients with a standard deviation of 0.018/cm. These coefficients facilitate the accurate prediction of wave numbers for the vibrational levels with v-prime and v-double prime between 0 and 4.

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