Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-24T14:06:36.770Z Has data issue: false hasContentIssue false
  • English
  • Français

A systematic and detailed investigation of radiative rates for forbidden transitions of astrophysical interest in doubly ionized iron peak elements

Published online by Cambridge University Press:  18 July 2017

Pascal Quinet ,
Vanessa Fivet  and
Manuel Bautista
Pascal Quinet
Affiliation:
Physique Atomique et Astrophysique, Université de Mons, B-7000, Mons, Belgium email: [email protected]
Vanessa Fivet
Affiliation:
Physique Atomique et Astrophysique, Université de Mons, B-7000, Mons, Belgium email: [email protected]
Manuel Bautista
Affiliation:
Dept. of Physics, Western Michigan University, Kalamazoo, MI 49008, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We carried out a systematic study of the electronic structure of doubly-ionized Fe-peak species, from Sc III to Ni III. The magnetic dipole (M1) and electric quadrupole (E2) transition probabilities were computed using the pseudo-relativistic Hartree-Fock (HFR) method and the central Thomas-Fermi-Dirac-Amaldi potential approximation implemented in the AUTOSTRUCTURE code. This multi-platform approach allowed for consistency checks and intercomparison and has proven very useful in many previous works for estimating the uncertainties affecting the radiative data.

Keywords

atomic dataatomic processes
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E12
Copyright
Copyright © International Astronomical Union 2017