Experimental and theoretical studies of DyIII: radiative lifetimes and oscillator strengths of astrophysical interest
(2002) In Monthly Notices of the Royal Astronomical Society 334(1). p.1-10- Abstract
- The lifetimes of three short-lived levels belonging to the 4f(9) 6p configuration and of two long-lived levels of the 4f(9) 5d configuration of Dy iii have been measured for the first time using time-resolved laser-induced fluorescence techniques. They are in good agreement with theoretical values calculated within the framework of a pseudo-relativistic configuration interaction approximation. Using the experimental lifetimes and the theoretical branching fractions, a first set of transition probabilities of astrophysical interest has been obtained for Dy III.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/333647
- author
- Zhang, Zhiguo ; Svanberg, Sune LU ; Palmeri, P ; Quinet, P and Biemont, E
- organization
- publishing date
- 2002
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- chemically peculiar, atomic data, stars :, atomic processes, techniques : spectroscopic
- in
- Monthly Notices of the Royal Astronomical Society
- volume
- 334
- issue
- 1
- pages
- 1 - 10
- publisher
- Oxford University Press
- external identifiers
-
- wos:000176834400003
- ISSN
- 1365-2966
- language
- English
- LU publication?
- yes
- id
- 81b015ee-08f5-44e3-a9b3-7306c3c388db (old id 333647)
- alternative location
- http://adsabs.harvard.edu/full/2002MNRAS.334....1Z
- date added to LUP
- 2016-04-01 12:01:02
- date last changed
- 2018-11-21 20:02:51
@article{81b015ee-08f5-44e3-a9b3-7306c3c388db, abstract = {{The lifetimes of three short-lived levels belonging to the 4f(9) 6p configuration and of two long-lived levels of the 4f(9) 5d configuration of Dy iii have been measured for the first time using time-resolved laser-induced fluorescence techniques. They are in good agreement with theoretical values calculated within the framework of a pseudo-relativistic configuration interaction approximation. Using the experimental lifetimes and the theoretical branching fractions, a first set of transition probabilities of astrophysical interest has been obtained for Dy III.}}, author = {{Zhang, Zhiguo and Svanberg, Sune and Palmeri, P and Quinet, P and Biemont, E}}, issn = {{1365-2966}}, keywords = {{chemically peculiar; atomic data; stars :; atomic processes; techniques : spectroscopic}}, language = {{eng}}, number = {{1}}, pages = {{1--10}}, publisher = {{Oxford University Press}}, series = {{Monthly Notices of the Royal Astronomical Society}}, title = {{Experimental and theoretical studies of DyIII: radiative lifetimes and oscillator strengths of astrophysical interest}}, url = {{https://lup.lub.lu.se/search/files/2744997/2371295.pdf}}, volume = {{334}}, year = {{2002}}, }