Oscillator strengths for transitions to Rydberg levels in 12C 16O, 13C 16O and 13C 18O between 967 and 972 Å - Faculté des Sciences de Sorbonne Université Accéder directement au contenu
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2004

Oscillator strengths for transitions to Rydberg levels in 12C 16O, 13C 16O and 13C 18O between 967 and 972 Å

Résumé

Absorption oscillator strengths have been determined from high-resolution spectra in the 967-972 Å region of three CO isotopomers for transitions to the Rydberg levels 4ppi(0), 3dpi(1)b and 4psigma(0), as well as to the mixed E(6) level recently characterized by Eidelsberg et al. (\cite{Eid04}). Synchrotron radiation from the Super-ACO electron storage ring at Orsay (LURE) was used as a light source. Oscillator strengths were extracted from the recorded spectra by least-squares fitting of the experimental profiles with synthetic spectra taking into account the homogeneous and heterogeneous interactions of the four levels. Column densities were derived from fits to the 3ppi(0) absorption band whose oscillator strength is well established. These are the first reported measurements for 13C18O. For 12C16Op, our results are consistent with the larger values obtained in the most recent laboratory and astronomical studies.
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hal-03786672 , version 1 (25-09-2022)

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Michèle Eidelsberg, Jean-Louis Lemaire, Jean-Hugues Fillion, Francois Rostas, S. R. Federman, et al.. Oscillator strengths for transitions to Rydberg levels in 12C 16O, 13C 16O and 13C 18O between 967 and 972 Å. Astronomy and Astrophysics - A&A, 2004, 424, pp.355-361. ⟨10.1051/0004-6361:20041017⟩. ⟨hal-03786672⟩
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