Journal article

Dielectronic recombination plasma rate coefficients of Na-, Mg-, and Al-like iron ions: The role of the 2(s + p) → 4l, nl′ and 3(s + p) → 5l, nl′ resonances


Authors listVisentin, G.; Schippers, S.; Fritzsche, S.

Publication year2023

JournalAstronomy & Astrophysics

Volume number679

ISSN0004-6361

eISSN1432-0746

Open access statusHybrid

DOI Linkhttps://doi.org/10.1051/0004-6361/202347456

PublisherEDP Sciences


Abstract
Dielectronic recombination (DR) is the major electron-ion recombination process in many astrophysical and laboratory plasmas. This process has been thoroughly studied for several charged species, in particular for M-shell iron ions. Previous investigations into the DR of such ions have mostly focused on the valence 3l -> 3l, nl' and the core 2(s + p) -> 3l, nl ' DR resonances, while neglecting the 2(s + p) -> 4l, nl ' and 3(s + p) -> 5l, nl ' DR resonances. These were predicted to contribute to the broad unresolved transition array detected in several active galactic nuclei at reasonably high temperatures and column densities. In this work, we systematically assessed the importance of 2(s + p) -> 4l, nl ' and 3(s + p) -> 5l, nl ' resonances in the DR of three M-shell iron ions, Fe15+, Fe14+, and Fe13+, with the multi-configuration Dirac-Hartree-Fock (MCDHF) method. Above the collisionally ionized plasma temperatures, these high-energy resonances contribute to the overall DR of Fe15+, Fe14+, and Fe13+ by up to 21%, 40%, and 22%, respectively.



Citation Styles

Harvard Citation styleVisentin, G., Schippers, S. and Fritzsche, S. (2023) Dielectronic recombination plasma rate coefficients of Na-, Mg-, and Al-like iron ions: The role of the 2(s + p) → 4l, nl′ and 3(s + p) → 5l, nl′ resonances, Astronomy & Astrophysics, 679, Article A13. https://doi.org/10.1051/0004-6361/202347456

APA Citation styleVisentin, G., Schippers, S., & Fritzsche, S. (2023). Dielectronic recombination plasma rate coefficients of Na-, Mg-, and Al-like iron ions: The role of the 2(s + p) → 4l, nl′ and 3(s + p) → 5l, nl′ resonances. Astronomy & Astrophysics. 679, Article A13. https://doi.org/10.1051/0004-6361/202347456



Keywords


ATOMIC DATAatomic processesFINITE-DENSITY PLASMASIONIZED-GASLABORATORY MEASUREMENTSNUCLEAR ENVIRONMENTPlasmasrelativistic processesXMM-NEWTONX-RAY-ABSORPTION

Last updated on 2025-10-06 at 11:59