The Kα resonance complexes in oxygen ions O I-O VI are theoretically computed, and resonance oscillator strengths and wavelengths are presented. The highly resolved photoionization cross-sections, with relativistic fine structure, are computed in the coupled channel approximation using the Breit-Pauli R-matrix method. A number of strong Kα resonances are found to be appreciable, with resonance oscillator strengths fr > 0.1. The Kα resonance wavelengths of O I-O VI lie in the relatively narrow wavelength range 22-23.5 Å, and the X-ray opacity in this region should therefore be significantly affected by K → L transitions in oxygen. The results should be useful in the interpretation of soft X-ray spectra observed from Chandra and XMM-Newton.
CITATION STYLE
Pradhan, A. K., Xin Chen, G., Delahaye, F., Nahar, S. N., & Oelgoetz, J. (2003). X-ray absorption via Kα resonance complexes in oxygen ions. Monthly Notices of the Royal Astronomical Society, 341(4), 1268–1271. https://doi.org/10.1046/j.1365-8711.2003.06513.x
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