Emission spectra with a high resolution Fourier transform spectrometer: CO spectra and their astrophysical importance

Details Emission spectra with a high resolution Fourier transform spectrometer: CO spectra and their astrophysical importance Emission spectra with a high resolution Fourier transform spectrometer: CO spectra and their astrophysical importance

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974jmosp..53..466m&link_type=abstract

Journal of Molecular Spectroscopy, Volume 53, Issue 3, p. 466-478.

Physics

17

Scientific paper

Line positions and molecular constants are reported for the 2-0, 3-1, 4-2, 5-3, 6-4, and 7-5 bands of CO observed in emission. The absolute uncertainty of unblended line positions is on the order of +/-0.0003 cm-1.
High resolution stellar, sunspot, and laser spectra (for v <= 7, J < 100) are calculated to within the experimental uncertainty of the published data using the molecular constants derived in this study.
Permanent address: Observatoire de Meudon, Laboratoire du Télescope Infra-Rouge, 1, Place Jules Janssen, 92190, Meudon, France.

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