Fourier spectroscopy of the C-12C-13 and /C-13/2 Ballik-Ramsay system

Details Fourier spectroscopy of the C-12C-13 and /C-13/2 Ballik-Ramsay system Fourier spectroscopy of the C-12C-13 and /C-13/2 Ballik-Ramsay system

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...263..993a&link_type=abstract

Astrophysical Journal, Part 1, vol. 263, Dec. 15, 1982, p. 993-998.

Astronomy and Astrophysics

Astrophysics

10

Carbon Stars, Fourier Analysis, Molecular Spectroscopy, Stellar Atmospheres, Atomic Structure, Carbon 12, Carbon 13, Data Reduction, Emission Spectra, Environmental Laboratories, Interferometry, Least Squares Method, Spectral Resolution, Vibrational Spectra

Scientific paper

Experimental observations and analyses of the Ballik-Ramsay electronic system of C-13 are reported. C2 emission spectra were obtained using a microwave discharge in a sealed tube filled with two isotopic volumes of CO gas to produce a C-12C-13 molecule. Fourier interferometry was employed to record in the spectral range 3500-14,000/cm, with a resolution limit of 0.013/cm. An iterative, nonlinear, least squares method was used to reduce the observed wavenumbers for the 0-0 band to molecular parameters.

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