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 (Feâ XVII-Feâ XXV)

Deprince J, Bautista MA, Fritzsche S, Garcia J, Kallman T, Mendoza C, Palmeri P, Quinet P (2019)


Publication Type: Journal article

Publication year: 2019

Journal

Book Volume: 626

Article Number: A83

DOI: 10.1051/0004-6361/201935444

Abstract

Aims. In the context of accretion disks around black holes, we estimate plasma-environment effects on the atomic parameters associated with the decay of K-vacancy states in highly charged iron ions, namely Feâ XVII-Feâ XXV. Methods. Within the relativistic multiconfiguration Dirac-Fock (MCDF) framework, the electron-nucleus and electron-electron plasma screenings were approximated with a time-Averaged Debye-Hückel potential. Results. Modified ionization potentials, K thresholds, wavelengths, radiative emission rates, and Auger widths are reported for astrophysical plasmas characterized by electron temperatures and densities in the ranges 105â-Â 107 K and 1018â-Â 1022 cm-3, respectively. Conclusions. We conclude that the high-resolution microcalorimeters on board future X-ray missions such as XRISM and ATHENA are expected to be sensitive to the lowering of the iron K edge due to the extreme plasma conditions occurring in accretion disks around compact objects.

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APA:

Deprince, J., Bautista, M.A., Fritzsche, S., Garcia, J., Kallman, T., Mendoza, C.,... Quinet, P. (2019). 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 (Feâ XVII-Feâ XXV). Astronomy & Astrophysics, 626. https://doi.org/10.1051/0004-6361/201935444

MLA:

Deprince, Jerome, et al. "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 (Feâ XVII-Feâ XXV)." Astronomy & Astrophysics 626 (2019).

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