2020A&A...643A..57D


Query : 2020A&A...643A..57D

2020A&A...643A..57D - Astronomy and Astrophysics, volume 643A, 57-57 (2020/11-1)

Plasma environment effects on K lines of astrophysical interest. IV. IPs, K thresholds, radiative rates, and Auger widths in Fe II-Fe VIII.

DEPRINCE J., BAUTISTA M.A., FRITZSCHE S., GARCIA J.A., KALLMAN T.R., MENDOZA C., PALMERI P. and QUINET P.

Abstract (from CDS):


Aims. Within the framework of compact-object accretion disks, we calculate plasma environment effects on the atomic structure and decay parameters used in the modeling of K lines in lowly charged iron ions, namely FeII-FeVIII.
Methods. For this study, we used the fully relativistic multiconfiguration Dirac-Fock 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 105-107K and 1018-1022cm–3. In addition, we propose two universal fitting formulae to predict the IP and K-threshold lowerings in any elemental ion.
Conclusions. We conclude that the high-resolution X-ray spectrometers onboard the future XRISM and ATHENA space missions will be able to detect the lowering of the K edges of these Fe ions due to the extreme plasma conditions occurring in the accretion disks around compact objects.

Abstract Copyright: © ESO 2020

Journal keyword(s): black hole physics - plasmas - atomic data - X-rays: general

VizieR on-line data: <Available at CDS (J/A+A/643/A57): table4.dat>

Simbad objects: 0

goto Full paper

goto View the references in ADS

Number of rows : 0

To bookmark this query, right click on this link: simbad:objects in 2020A&A...643A..57D and select 'bookmark this link' or equivalent in the popup menu