Dielectronic Recombination of Fe XV forming Fe XIV: Laboratory Measurements and Theoretical Calculations
arXiv:0704.0905 · doi:10.1086/519073
Abstract
We have measured resonance strengths and energies for dielectronic recombination (DR) of Mg-like Fe XV forming Al-like Fe XIV via N=3 -> N' = 3 core excitations in the electron-ion collision energy range 0-45 eV. All measurements were carried out using the heavy-ion Test Storage Ring at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We have also carried out new multiconfiguration Breit-Pauli (MCBP) calculations using the AUTOSTRUCTURE code. For electron-ion collision energies < 25 eV we find poor agreement between our experimental and theoretical resonance energies and strengths. From 25 to 42 eV we find good agreement between the two for resonance energies. But in this energy range the theoretical resonance strengths are ~ 31% larger than the experimental results. This is larger than our estimated total experimental uncertainty in this energy range of +/- 26% (at a 90% confidence level). Above 42 eV the difference in the shape between the calculated and measured 3s3p(^1P_1)nl DR series limit we attribute partly to the nl dependence of the detection probabilities of high Rydberg states in the experiment. We have used our measurements, supplemented by our AUTOSTRUCTURE calculations, to produce a Maxwellian-averaged 3 -> 3 DR rate coefficient for Fe XV forming Fe XIV. The resulting rate coefficient is estimated to be accurate to better than +/- 29% (at a 90% confidence level) for k_BT_e > 1 eV. At temperatures of k_BT_e ~ 2.5-15 eV, where Fe XV is predicted to form in photoionized plasmas, significant discrepancies are found between our experimentally-derived rate coefficient and previously published theoretical results. Our new MCBP plasma rate coefficient is 19-28% smaller than our experimental results over this temperature range.
References in corpus (25)
- The Ionized Gas and Nuclear Environment in NGC 3783. I. Time-Averaged 900 ks Chandra Grating Spectroscopy
- Dielectronic recombination data for dynamic finite-density plasmas I. Goals and methodology
- The Ionized Gas and Nuclear Environment in NGC 3783. IV. Variability and Modeling of the 900 ks CHANDRA Spectrum
- Complex resonance absorption structure in the X-ray spectrum of IRAS13349+2438
- Soft X-Ray Absorption by Fe to Fe in Active Galactic Nuclei
- A Long Look at NGC 3783 with the XMM-Newton Reflection Grating Spectrometers
- XMM-NEWTON High Resolution Spectroscopy of NGC 5548
- Storage ring measurement of the C IV recombination rate coefficient
- Exploring the complex X-ray spectrum of NGC 4051
- Multi-wavelength study of the Seyfert 1 galaxy NGC 3783 with XMM-Newton
- An XMM-Newton observation of the luminous Seyfert 1 galaxy Markarian 509
- Dielectronic recombination of Fe 3p^q ions: a key ingredient for describing X-ray absorption in active galactic nuclei
- The Iron Unresolved Transition Array in Active Galactic Nuclei
- Dielectronic Recombination in Photoionized Gas. II. Laboratory Measurements for Fe XVIII and Fe XIX
- Experimental Mg IX photorecombination rate coefficient
- The Ionized Nuclear Environment in NGC 985 as seen by Chandra and BeppoSAX
- Interference effects in the photorecombination of argonlike Sc3+ ions: Storage-ring experiment and theory
- Dielectronic recombination of lithium-like Ni25+ ions - high resolution rate coefficients and influence of external crossed E and B fields
- Dielectronic Recombination (via N=2 --> N'=2 Core Excitations) and Radiative Recombination of Fe XX: Laboratory Measurements and Theoretical Calculations
- The Effects of Low-Temperature Dielectronic Recombination on the Relative Populations of the Fe M-Shell States
- Electron-ion recombination measurements motivated by AGN X-ray absorption features: Fe XIV forming Fe XIII
- IZw1 observed with XMM-Newton: Low-energy spectral complexity, iron lines, and hard X-ray flares
- The Properties and the Evolution of the Highly Ionized Gas in MR2251-178
- Dielectronic recombination of Fe^{13+}: benchmarking the M-shell
- Experimentally Derived Dielectronic Recombination Rate Coefficients for Heliumlike C V and Hydrogenic O VIII
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- The Impact of Recent Advances in Laboratory Astrophysics on our Understanding of the Cosmos
- Polarization of K-shell dielectronic recombination satellite lines of Fe XIX-XXV and its application for diagnostics of anisotropies of hot plasmas
- Astrophysical Relevance of Storage-Ring Electron-Ion Recombination Experiments
- Electron-ion Recombination of Fe X forming Fe IX and of Fe XI forming Fe X: Laboratory Measurements and Theoretical Calculations
- Electron-ion recombination of Si IV forming Si III: Storage-ring measurement and multiconfiguration Dirac-Fock calculations
- Dielectronic Recombination of Argon-Like Ions
- Absolute rate coefficients for photorecombination and electron-impact ionization of magnesium-like iron ions from measurements at a heavy-ion storage ring
- Spectral Implications of Atomic Uncertainties in Optically-thin Hot Plasmas
- Resonant Electron Impact Excitation of 3d levels in Fe and Fe