An investigation of oscillator strength calculations for interstellar lines of CL I

Details An investigation of oscillator strength calculations for interstellar lines of CL I An investigation of oscillator strength calculations for interstellar lines of CL I

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p..52k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 15, 1990, p. 52P-54P. Research supported by S

Astronomy and Astrophysics

Astronomy

7

Astronomical Spectroscopy, Chlorine, Interstellar Gas, Line Spectra, Oscillator Strengths, Absorption Spectra, Electron Transitions, Interstellar Extinction, Ultraviolet Spectra

Scientific paper

Recent oscillator strength calculations for the 1088.062, 1097.369 and 1347.240 A interstellar lines of Cl I by Ojha and Hibbert (1990) are found to be incompatible with high quality Copernicus observations. Possible explanations are discussed, including severe blending in the observational data, and misidentification of the 1088.062 and 1097.369 A transitions. Until these discrepancies are resolved, column densities deduced from these two transitions should be treated with caution.

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