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Oscillator strengths for lines of astrophysical interest in Rh II

Quinet, P. (author)
Astrophysique et Spectroscopie, Université de Mons – UMONS, 7000 Mons, Belgium; IPNAS, Université de Liège, Sart Tilman, 4000 Liège, Belgium
Biémont, E. (author)
Astrophysique et Spectroscopie, Université de Mons – UMONS, 7000 Mons, Belgium; IPNAS, Université de Liège, Sart Tilman, 4000 Liège, Belgium
Palmeri, P. (author)
Astrophysique et Spectroscopie, Université de Mons – UMONS, 7000 Mons, Belgium
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Engström, L. (author)
Department of Physics, Lund University, PO Box 118, 221 00 Lund, Swede
Hartman, H. (author)
Lund Observatory, Lund University, PO Box 43, 221 00 Lund, Sweden
Lundberg, H. (author)
Department of Physics, Lund University, PO Box 118, 221 00 Lund, Swede
Nilsson, H. (author)
Lund Observatory, Lund University, PO Box 43, 221 00 Lund, Sweden
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 (creator_code:org_t)
2012-01-11
2012
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 537, s. A74-A74
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Aims. This work reports oscillator strengths for transitions of astrophysical interest in singly ionized rhodium.Methods. Seventeen radiative lifetimes in Rh+ have been measured with the time-resolved laser-induced fluorescence technique and combined with theoretical branching fractions calculated using a relativistic Hartree-Fock model including core-polarization effects to obtain oscillator strengths.Results. On the basis of the good agreement between theory and experiment for the lifetimes, new reliable oscillator strengths have been deduced for a set of 113 Rh II transitions in the spectral range 153–418 nm. 

Subject headings

NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

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