Atomic data for VUV lines of astrophysical interest in singly ionized rhodium
Quinet, P. ; Biemont, E. ; Palmeri, P. ; Engström, Lars LU ; Hartman, Henrik LU
; Lundberg, Hans
LU
and Nilsson, Hampus
LU
(2011)
In Journal of Electron Spectroscopy and Related Phenomena
184(3-6).
p.174-176
- 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.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/2032257
- author
- Quinet, P.
; Biemont, E.
; Palmeri, P.
; Engström, Lars
LU
; Hartman, Henrik
LU
; Lundberg, Hans
LU
and Nilsson, Hampus
LU
- organization
- publishing date
- 2011
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- Electronic structure, Oscillator strengths, Transition probabilities, Radiative lifetimes
- in
- Journal of Electron Spectroscopy and Related Phenomena
- volume
- 184
- issue
- 3-6
- pages
- 174 - 176
- publisher
- Elsevier
- external identifiers
-
- wos:000292173400019
- scopus:79957591699
- ISSN
- 0368-2048
- DOI
- 10.1016/j.elspec.2010.08.001
- language
- English
- LU publication?
- yes
- id
- dbe135cd-4f1f-45d7-a2fa-1a46db5c390b (old id 2032257)
- date added to LUP
- 2016-04-01 13:59:56
- date last changed
- 2024-01-09 21:41:47
@article{dbe135cd-4f1f-45d7-a2fa-1a46db5c390b,
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.}},
author = {{Quinet, P. and Biemont, E. and Palmeri, P. and Engström, Lars and Hartman, Henrik and Lundberg, Hans and Nilsson, Hampus}},
issn = {{0368-2048}},
keywords = {{Electronic structure; Oscillator strengths; Transition probabilities; Radiative lifetimes}},
language = {{eng}},
number = {{3-6}},
pages = {{174--176}},
publisher = {{Elsevier}},
series = {{Journal of Electron Spectroscopy and Related Phenomena}},
title = {{Atomic data for VUV lines of astrophysical interest in singly ionized rhodium}},
url = {{http://dx.doi.org/10.1016/j.elspec.2010.08.001}},
doi = {{10.1016/j.elspec.2010.08.001}},
volume = {{184}},
year = {{2011}},
}