Absolute transition probabilities in the spectra of EU II. III - Astrophysical applications

Details Absolute transition probabilities in the spectra of EU II. III - Astrophysical applications Absolute transition probabilities in the spectra of EU II. III - Astrophysical applications

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...107..166b&link_type=abstract

Astronomy and Astrophysics, vol. 107, no. 1, Mar. 1982, p. 166-171. Research supported by the Fonds National de la Recherche Sc

Astronomy and Astrophysics

Astrophysics

102

Europium, Photosphere, Solar Atmosphere, Solar Spectra, Stellar Spectra, Transition Probabilities, Abundance, Chemical Composition, Iron, Line Spectra, Nuclear Fusion

Scientific paper

Astrophysical implications of a new scale of accurate oscillator
strengths obtained for Eu II are discussed. A new value of the solar
photospheric abundance of Europium is derived: A(Eu) equals 0.51 plus or
minus 0.08, in the usual logarithmic scale. Some stellar implications of
the new gf-values are also presented.

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