Improved atomic data for iridium atom (Ir I) and ion (Ir II) and the solar content of iridium
(2007) In Journal of Quantitative Spectroscopy and Radiative Transfer 104. p.52-70- Abstract
- From a combination of radiative lifetime measurements, performed with a time-resolved laser-induced fluorescence technique, for nine odd-parity levels of Ir I and four odd-parity levels of Ir II and branching fraction calculations, extended sets of transition probabilities have been derived for transitions of astrophysical interest. The new results are compared with the few experimental data available in the literature and a good agreement is found. They extend considerably the previous sets of transition probabilities available in the literature. Implications of the new results regarding the solar content of iridium are briefly discussed.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/796219
- author
- Xu, Huailiang LU ; Svanberg, Sune LU ; Quinet, Pascal ; Palmeri, P. and Biemont, Emile
- organization
- publishing date
- 2007
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Journal of Quantitative Spectroscopy and Radiative Transfer
- volume
- 104
- pages
- 52 - 70
- publisher
- Elsevier
- external identifiers
-
- wos:000242758700005
- scopus:33750514185
- ISSN
- 0022-4073
- DOI
- 10.1016/j.jqsrt.2006.08.010
- language
- English
- LU publication?
- yes
- id
- 3e328f36-bd59-44eb-9ad7-27d6b9b0da07 (old id 796219)
- date added to LUP
- 2016-04-04 14:38:16
- date last changed
- 2022-03-16 03:47:16
@article{3e328f36-bd59-44eb-9ad7-27d6b9b0da07, abstract = {{From a combination of radiative lifetime measurements, performed with a time-resolved laser-induced fluorescence technique, for nine odd-parity levels of Ir I and four odd-parity levels of Ir II and branching fraction calculations, extended sets of transition probabilities have been derived for transitions of astrophysical interest. The new results are compared with the few experimental data available in the literature and a good agreement is found. They extend considerably the previous sets of transition probabilities available in the literature. Implications of the new results regarding the solar content of iridium are briefly discussed.}}, author = {{Xu, Huailiang and Svanberg, Sune and Quinet, Pascal and Palmeri, P. and Biemont, Emile}}, issn = {{0022-4073}}, language = {{eng}}, pages = {{52--70}}, publisher = {{Elsevier}}, series = {{Journal of Quantitative Spectroscopy and Radiative Transfer}}, title = {{Improved atomic data for iridium atom (Ir I) and ion (Ir II) and the solar content of iridium}}, url = {{https://lup.lub.lu.se/search/files/6406319/2371285.pdf}}, doi = {{10.1016/j.jqsrt.2006.08.010}}, volume = {{104}}, year = {{2007}}, }