Infrared bands of C2 in the solar photospheric spectrum

Details Infrared bands of C2 in the solar photospheric spectrum Infrared bands of C2 in the solar photospheric spectrum

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..201b&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 201-205. Research supported by the Fonds de la Recherche Fondamental

Astronomy and Astrophysics

Astronomy

39

Carbon, Infrared Spectra, Photosphere, Solar Spectra, Spectral Bands, High Resolution, Infrared Astronomy, Molecular Oscillations, Solar Atmosphere, Solar Physics, Spectrum Analysis, Stellar Spectrophotometry

Scientific paper

Lines of the C2 Phillips system have been successfully searched for on new tracings of high resolution solar spectra. From a rather large number of lines of the (0,0), (1,0), and (0, 1) bands, we derive empirical values for the band oscillator strengths: f00 = 1.41 10-3, f10 = 1.38 10-3, and f01 = 1.12 10-3. These solar f-values are discussed in section 3.1 and compared with recent laboratory data.
For the Ballik-Ramsay system, only a few unblended solar lines have been available, from which we deduced 0.6 10-3 ≪ f00 ≪ 1.2 10-3.

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