Theoretical oscillator strengths of some transitions of Y II and Zr II

Details Theoretical oscillator strengths of some transitions of Y II and Zr II Theoretical oscillator strengths of some transitions of Y II and Zr II

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72...55p&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 55-59.

Astronomy and Astrophysics

Astrophysics

5

Abundance, Astrophysics, Electron Transitions, Molecular Oscillators, Yttrium, Zirconium, Thomas-Fermi Model

Scientific paper

The gf-values of some transitions of Y II and Zr II are calculated to
test the reliability of values commonly used in astrophysical
applications. The astrophysical interest of these transitions is
associated with the determination of the solar abundance of Y and Zr and
with the analysis of the Sr-Y-Zr peak in Ap and Bp stars.

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