Oscillator strengths for lines of astrophysical interest in Rh II

Details Oscillator strengths for lines of astrophysical interest in Rh II Oscillator strengths for lines of astrophysical interest in Rh II

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012a%26a...537a..74q&link_type=abstract

Astronomy & Astrophysics, Volume 537, id.A74

Astronomy and Astrophysics

Astrophysics

Atomic Processes, Atomic Data

Scientific paper

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.
Table 3 is also available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/537/A74

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