Multiconfiguration Dirac-Hartree-Fock energy levels and transition probabilities for 3d^5 in Fe IV
arXiv:0809.4720 · doi:10.1111/j.1365-2966.2008.13997.x
Abstract
Multiconfiguration Dirac-Hartree-Fock electric quadrupole (E2) and magnetic dipole (M1) transition probabilities are reported for transitions between levels of 3d^5 in [Fe IV]. The accuracy of the ab initio energy levels and the agreement in the length and velocity forms of the line strength for the E2 transitions are used as indicators of accuracy. The present E2 and M1 transition probabilities are compared with earlier Breit-Pauli results and other theories. An extensive set of transition probabilites with indicators of accuracy are reported in Appendices A and B. Recommended values of A(E2) + A(M1) are listed in Appendix C.
16 pages, three appendices containing accuracy indicators and recommended values for E2 and M1 transition rates
References in corpus (3)
Cited by in corpus (13)
- Keck HIRES Spectroscopy of Extragalactic HII Regions: C and O Abundances from Recombination Lines
- NGC 2579 and the carbon and oxygen abundance gradients beyond the solar circle
- Near L-Edge Single and Multiple Photoionization of Singly Charged Iron Ions
- C/O abundance ratios, iron depletions, and infrared dust features in Galactic planetary nebulae
- S-process enrichment in the planetary nebula NGC 3918. Results from deep echelle spectrophotometry
- Forbidden Iron Lines and Dust Destruction in Supernova Remnant Shocks: The Case of N49 in the Large Magellanic Cloud
- Near L-edge photoionization of triply charged iron ions
- C/O ratios in planetary nebulae with dual-dust chemistry from faint optical recombination lines
- The homogeneity of chemical abundances in H II regions of the Magellanic Clouds
- Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy I: HH529II and III
- Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy II: HH204
- Gas-phase Fe/O and Fe/N abundances in Star-Forming Regions. Relations between nucleosynthesis, metallicity and dust
- Irreducible tensor-form of the relativistic corrections to the M1 transition operator