The optically thick O III spectrum. I - Diagnostic ratios involving the intercombination lines

Statistics – Computation

Scientific paper

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Astronomical Photometry, Optical Thickness, Oxygen Spectra, Ultraviolet Spectra, Computational Astrophysics, Electron Transitions, Iue, Resonance Lines

Scientific paper

An escape-probability calculation of the optically thick O III spectrum is carried out to obtain the optical depth dependence of the intercombination doublet at 1663 A and of resonance lines between the 2p2, 2s2p3, and 2p4 configurations. The effect of optical depth on diagnostic ratios involving the intercombination lines is quantitatively established. The general question raised is whether such effects may occur in actual sources.

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