Oscillator Strengths for Neutral Carbon Lines below 1200 Å

Physics

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Scientific paper

We analyzed high resolution spectra of interstellar absorption from C I toward δ Sco, λ Ori, and 1 Sco, obtained with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. Several multiplets were detected within the wavelength interval 1150-1200 Åwhere most C I lines have ill-defined oscillator strength; multiplets at longer wavelengths with well-defined atomic parameters were also seen. We extracted accurate column densities and Doppler parameters from lines with precise laboratory-based f-values. These column densities and b-values were used to obtain a self-consistent set of f-values for all the observed C I lines. For almost all lines with wavelength below 1200 Åthe derived f-values differ appreciably from the values quoted in the compilation by Morton (1991).

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