Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210..439c&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Sept. 15, 1984, p. 439-442.
Astronomy and Astrophysics
Astronomy
8
Atomic Spectra, Configuration Interaction, Heavy Ions, Oscillator Strengths, Solar Spectra, Spin-Orbit Interactions, Atomic Structure, Integral Equations, Iron, Resonance Lines, Ultraviolet Spectra, Wavelengths
Scientific paper
The authors re-emphasize the importance of both spin-orbit interaction and configuration-mixing effects in the calculation of wavelengths and oscillator stengths for heavy-element moderately-ionized spectra; with particular reference to Fe X resonance lines. They correct several rather misleading statements in a recent paper by R. Glass on Fe X, and dispute the argument that three- and four-electron correlation effects are important. They discuss afresh the (well-established) method of allowing for weak correlations by the scaling of radial integrals, and consider its implications for oscillator stength calculations.
Bromage Gordon E.
Cowan Robert D.
Fawcett B. C.
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