Abstract
The first theoretical transition probabilities and oscillator strengths are reported for Rh II lines of astrophysical interest in the VUV region (100-200 nm). They have been obtained through the use of a pseudo-relativistic Hartree-Fock model including core-polarization effects and the accuracy has been estimated to be about 10-15% through a comparison with new experimental lifetimes measured using the time-resolved laser-induced fluorescence technique. (C) 2010 Elsevier B.V. All rights reserved.
Original language | English |
---|---|
Pages (from-to) | 174-176 |
Journal | Journal of Electron Spectroscopy and Related Phenomena |
Volume | 184 |
Issue number | 3-6 |
DOIs | |
Publication status | Published - 2011 |
Subject classification (UKÄ)
- Astronomy, Astrophysics and Cosmology
- Atom and Molecular Physics and Optics
Free keywords
- Electronic structure
- Oscillator strengths
- Transition probabilities
- Radiative lifetimes