Radiative lifetime measurements and oscillator strengths of astrophysical interest in HoIII
Author
Summary, in English
Radiative lifetimes of three long-lived levels belonging to the 4f(10)5d configuration of Ho III have been measured, for the first time, using the time-resolved laser-induced fluorescence technique. A good agreement between the experimental lifetimes and theoretical results obtained within a multiconfigurational pseudo-relativistic Hartree-Fock (HFR) approach including core-polarization (CP) effects is observed provided an adequate scaling factor is applied to the <4f&VERBAR;r&VERBAR;5d> transition matrix element. From the comparison theory-experiment, it has been possible to assess the reliability of the oscillator strengths of the 4f-5d transitions of astrophysical interest, particularly for the lines depopulating the levels considered in the present work. The present results fill in a gap concerning the f-values of doubly ionized holmium and are needed for a quantitative evaluation of the holmium abundance in some peculiar stars.
Department/s
Publishing year
2002
Language
English
Pages
364-370
Publication/Series
Astronomy & Astrophysics
Volume
384
Issue
1
Full text
- Available as PDF - 140 kB
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Document type
Journal article
Publisher
EDP Sciences
Topic
- Atom and Molecular Physics and Optics
Keywords
- atomic processes
- stars : chemically peculiar
- atomic data
Status
Published
ISBN/ISSN/Other
- ISSN: 0004-6361