On the determination of the solar iron abundance using Fe II lines

Details On the determination of the solar iron abundance using Fe II lines On the determination of the solar iron abundance using Fe II lines

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...340..300r&link_type=abstract

Astronomy and Astrophysics, v.340, p.300-304 (1998)

Astronomy and Astrophysics

Astrophysics

68

Atomic Data, Sun: Abundances

Scientific paper

Transition probabilities of lines related to odd terms based on the lowest ((5) D) parent of Fe ii have been calculated using the orthogonal operator approach for both the odd and the even energy levels. The obtained log(gf) values are used to calculate the solar Fe-abundance. The result, AFe = 7.59 +/- 0.06, is the average of the two abundance values proposed in recent literature. The full Table~\ref{tab1} is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html.

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