Published February 1, 2021 | Version v1
Journal article

Near L-edge Single and Multiple Photoionization of Doubly Charged Iron Ions

  • 1. I. Physikalisches Institut, Justus-Liebig-Universität Gießen, Heinrich-Buff-Ring 16, 35392 Giessen (Germany)
  • 2. Helmholtz-Institut Jena, Fröbelstieg 3, 07743 Jena (Germany)
  • 3. Deutsches Elektronen-Synchrotron DESY, Notkestrae 85, 22607 Hamburg (Germany)
  • 4. Advanced Light Source, MS 80RO114, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States)
  • 5. Department of Physics, University of Nevada, Reno, NV 89557-0220 (United States)
  • 6. Institut für Experimentalphysik, Universität Hamburg, Luruper Chaussee 149, 22761 Hamburg (Germany)
  • 7. Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, New York 10027 (United States)
  • 8. Institut für Atom- und Molekülphysik, Justus-Liebig-Universität Gießen, Leihgesterner Weg 217, 35392 Giessen (Germany)

Description

Using the photon–ion merged-beams technique at a synchrotron light source, we have measured relative cross sections for single and up to five-fold photoionization of Fe2+ ions in the energy range of 690–920 eV. This range contains thresholds and resonances associated with ionization and excitation of 2p and 2s electrons. Calculations were performed to simulate the total absorption spectra. The theoretical results show very good agreement with the experimental data, if overall energy shifts of up to 2.5 eV are applied to the calculated resonance positions and assumptions are made about the initial experimental population of the various levels of the Fe2+([Ar]3d 6) ground configuration. Furthermore, we performed extensive calculations of the Auger cascades that result when an electron is removed from the 2p subshell of Fe2+. These computations lead to a better agreement with the measured product-charge-state distributions as compared to earlier work. We conclude that the L-shell absorption features of low-charged iron ions are useful for identifying gas-phase iron in the interstellar medium and for discriminating against the various forms of condensed-phase iron bound to composite interstellar dust grains.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4357/abcc64

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
908
Journal Issue
1
Journal Page Range
[8 p.]
ISSN
0004-637X
CODEN
ASJOAB