On the establishment of internally consistent solar scales of oscillator strengths and abundances of chemical elements. III - Oscillator strengths obtained from equivalent widths of 360 FeI lines

Details On the establishment of internally consistent solar scales of oscillator strengths and abundances of chemical elements. III - Oscillator strengths obtained from equivalent widths of 360 FeI lines On the establishment of internally consistent solar scales of oscillator strengths and abundances of chemical elements. III - Oscillator strengths obtained from equivalent widths of 360 FeI lines

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...47..193g&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 47, Feb. 1982, p. 193-197.

Astronomy and Astrophysics

Astrophysics

22

Abundance, Fraunhofer Lines, Iron, Molecular Oscillators, Solar Spectra, Spectral Line Width, Molecular Excitation, Photosphere

Scientific paper

Oscillator strengths for 360 selected Fraunhofer lines were determined using the observed equivalent widths of those lines. The R.M.S. error of the gf-values obtained amounts to 0.06-0.07 dex. The comparison of oscillator strengths calculated from equivalent widths (w) and central intensity (d) shows the reliability of the methods used and of the underlaying data. The systematic increase of the difference log gfW - log gfd for strong lines of high excitation potential is noticeable.

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