Computer Science
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...20g&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Jan.-Feb. 1986, p. 20-23. In Russian.
Computer Science
1
Metallicity, Oscillator Strengths, Solar Spectra, Stellar Composition, Fraunhofer Lines, Line Spectra, Zirconium
Scientific paper
The oscillator strengths of 19 Zr I lines (rms error of + or 0.078 dex) and 10 Zr II lines (+ or - 0.081 dex) were determined from observed equivalent widths and central depths of solar Fraunhofer lines. An analysis of the differences between the oscillator strengths obtained from the equivalent widths and the central depths indicates that the Zr lines considered have no substantial hyperfine structure.
Gurtovenko Eh. A.
Kostyk R. I.
Orlova T. V.
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