Monthly Notices of the Royal Astronomical Society · 2003 · 36 citations · 26 references
Natural SciencesAstronomyChemistryRadiation PhysicsSpectroscopyX-ray AstronomyRadiation SpectroscopyX-ray SpectroscopyOpacityOpacity CalculationsOscillator StrengthsPhotoionization Cross SectionsSoft X-ray AstronomyX-ray Absorption SpectroscopyX-ray Emission LinesX-ray Spectra
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 ƒr > 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.
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RMATRX1: Belfast atomic R-matrix codes
K A Berrington, W. Eissner, P. H. Norrington · Computer Physics Communications · 1995 · 799 citations
Opacities for stellar envelopes
M. J. Seaton, Yu Yan, Dimitri Mihalas et al. · Monthly Notices of the Royal Astronomical Society · 1994 · 608 citations · Full text
Electron scattering by complex atoms
P. G. Burke, A Hibbert, W D Robb · Journal of Physics B Atomic and Molecular Physics · 1971 · 446 citations