Influence of Resonances on Spectral Formation of X-Ray Lines in Fe XVII
arXiv:astro-ph/0201513 · doi:10.1103/PhysRevLett.89.013202
Abstract
New theoretical results from large-scale relativistic close coupling calculations reveal the precise effect of resonances in collisional excitation of x-ray lines of Ne-like Fe XVII. Employing the Breit-Pauli R-matrix method and a 89-level eigenfunction expansion including up to n = 4 levels shows significant resonance enhancement of the collision strengths of forbidden and intercombination transitions. The present results differ from all previous calculations, heretofore without detailed resonance structures, and should help resolve longstanding discrepancies. In particular, the present line ratios of three benchmark diagnostic lines 3C, 3D, and 3E at 15.014, 15.265, and 15.456 A respectively, are in excellent agreement with two independent measurements on Electron-Beam-Ion-Traps [Laming et al, Astrophys. J, 545, L161 (2000) and Brown et al, Astrophys. J, 502, 1015 (1998)]. The strong energy dependence due to resonances in these and other cross sections is demonstrated for the first time. It is of general importance and strongly manifests itself in x-ray plasma diagnostics.
Phys. Rev. Letters (in press), 6 pages, 2 figures in color
Cited by in corpus (14)
- Atomic Data for X-ray Astrophysics
- Lower entropy bounds and particle number fluctuations in a Fermi sea
- Fe XVII X-ray Line Ratios for Accurate Astrophysical Plasma Diagnostics
- X-ray spectra of the Fe-L complex
- The Transparency of Solar Coronal Active Regions
- High Resolution Photoexcitation Measurements Exacerbate the Long-Standing Fe XVII Oscillator Strength Problem
- Breit-Pauli R-matrix calculations for electron impact excitation of Fe XVII: a benchmark study
- Revisiting the Fe XVII line emission problem: laboratory measurements of the 3s-2p and 3d-2p line-formation channels
- X-ray spectra of the Fe-L complex II: atomic data constraints from EBIT experiment and X-ray grating observations of Capella
- Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
- High-Precision Transition Energy Measurements of Neon-like Fe XVII Ions
- An XMM-Newton Study of the Coronae of Coronae Borealis
- Variation of the transition energies and oscillator strengths for the 3C and 3D lines of the Ne-like ions under plasma environment
- Fe XVII - line ratio diagnostic of shock formation radius in O stars