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Branching fractions and oscillator strengths for FeII transitions from the 3{ital d}{sup 6}({sup 5}{ital D})4{ital p} subconfiguration

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/177391· OSTI ID:286904
; ; ;  [1]; ;  [2]
  1. Physics Department, University of Wisconsin-Madison, Madison, Wisconsin 53706 (United States)
  2. Development of Physics, University of Lund, Soelvegatan 14, S-223 62 Lund (Sweden)

New experimental branching fractions and transition probabilities are reported for 56 transitions in FeII. The branching fractions are measured with a Fourier transform spectrometer and also with a high-resolution grating spectrometer on an optically thin hollow cathode discharge. Highly accurate experimental radiative lifetimes from the recent literature provide the normalization required to convert our branching fractions into absolute transition probabilities. Results are compared with experimental and theoretical values in the literature. Our new transition probabilities will establish the absolute scale for relative absorption oscillator strengths of vacuum ultraviolet lines measured using a new high-sensitivity absorption experiment at the University of Wisconsin. {copyright} {ital 1996 The American Astronomical Society.}

OSTI ID:
286904
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 464; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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