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Abstract
The configuration-interaction method as implemented in the computer code CIV3 is used to determine energy levels, electric dipole radiative transition wavelengths, oscillator strengths and transition probabilities for inner-shell excitation of transitions in Fe XV and Fe XVI. Specifically, transitions are considered of the type 1s22s22p63s2–1s22s22p53l3l′3l′′ (l, l′ and l′′= s, p or d) in Fe XV and 1s22s22p63s–1s22s22p53l3l′ (l and l′= s, p or d) in Fe XVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed.
Document Type
Article
Publication Date
2003
Digital Object Identifier (DOI)
http://dx.doi.org/10.1046/j.1365-8711.2003.06801.x
Repository Citation
Kisielius, R.; Hibbert, A.; Ferland, Gary J.; Foord, M. E.; Rose, S. J.; vanHoof, P. A. M.; and Keenan, F. P., "Inner-Shell Photoexcitation of Fe XV and Fe XVI" (2003). Physics and Astronomy Faculty Publications. 46.
https://uknowledge.uky.edu/physastron_facpub/46
Notes/Citation Information
Published in Monthly Notices of the Royal Astronomical Society, v. 344, issue 3, p. 696-706.
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2003 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
The copyright holder has granted the permission for posting the article here.