Plasma-environment effects on K lines of astrophysical interest III. IPs, K thresholds, radiative rates, and Auger widths in Fe ix - Fe xvi
arXiv:2001.11915 · doi:10.1051/0004-6361/201937088
Abstract
Aims. In the context of black-hole accretion disks, we aim to compute the plasma-environment effects on the atomic parameters used to model the decay of K-vacancy states in moderately charged iron ions, namely Fe ix - Fe xvi. Methods. We used the fully relativistic multiconfiguration Dirac-Fock (MCDF) method approximating the plasma electron-nucleus and electron-electron screenings with a time-averaged Debye-Huckel potential. Results. We report modified ionization potentials, K-threshold energies, wavelengths, radiative emission rates, and Auger widths for plasmas characterized by electron temperatures and densities in the ranges - K and - cm. Conclusions. This study confirms that the high-resolution X-ray spectrometers onboard the future XRISM and ATHENA space missions will be capable of detecting the lowering of the K edges of these ions due to the extreme plasma conditions occurring in accretion disks around compact objects.
arXiv comment6 pages, 5 figures, to be published in A&A
References in corpus (17)
- Improved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays
- X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
- The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
- X-ray reflected spectra from accretion disk models. I. Constant density atmospheres
- The Spin of Supermassive Black Holes
- Global Radiation Magneto-hydrodynamic Simulations of Sub-Eddington Accretion Disks around Supermassive Black Holes
- Modeling of iron K lines: radiative and Auger decay data for Fe II-Fe IX
- Alternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1
- High Density Reflection Spectroscopy: II. the Density of the Inner Black Hole Accretion Disc in AGN
- X-ray Spectra from MHD Simulations of Accreting Black Holes
- The Soft-Excess in Mrk 509: Warm Corona or Relativistic Reflection?
- Continuum Lowering -- A New Perspective
- High Density Reflection Spectroscopy I. A case study of GX~339-4
- Decay Properties of K-Vacancy States in Fe X-Fe XVII
- Reflection spectra from an accretion disc illuminated by a neutron star X-ray burst
- Plasma environment effects on K lines of astrophysical interest. II. Ionization potentials, K thresholds, radiative rates and Auger widths in Ne- through He-like iron ions (Fe xvii - Fe xxv)
- An Empirical Method for Improving the Quality of RXTE HEXTE Spectra