Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...396..715p&link_type=abstract
Astronomy and Astrophysics, v.396, p.715-722 (2002)
Astronomy and Astrophysics
Astrophysics
14
Atomic Data, Line: Identification, Techniques: Spectroscopic, Stars: Abundances, Ism: Abundances
Scientific paper
We report on experimental branching fractions (BFs) for 19 transitions from the three 3d5(6S)4s4p(3P) y6P levels in Fe II, measured in Fourier transform spectra of a Penning discharge lamp and a hollow cathode lamp. The transition wavelengths span the interval between 1600 and 2850 Å. Absolute oscillator strengths (f-values) have been derived by combining the BFs with experimental radiative lifetimes recently reported in the literature. Theoretical f-values have been calculated using configuration interaction wavefunctions. The new experimental and theoretical f-values are compared with data available in the literature and in databases. The strongest lines measured belong to the UV 8 multiplet of Fe II, which has one ground state transition appearing as a prominent feature at 1608 Å in interstellar spectra. The line is accompanied by a satellite at 1611 Å due to a level mixing, which is discussed in the paper.
Donnelly Marian Philomena
Hibbert Alan
Johansson Sara
Nilsson Hampus
Pickering Juliet C.
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