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Astron. Astrophys. 340, 300-304 (1998)


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

A.J.J. Raassen and P.H.M. Uylings

Van der Waals-Zeeman Instituut, Universiteit van Amsterdam, Valckenierstraat 65-67, 1018 XE Amsterdam, The Netherlands

Received 15 April 1998 / Accepted 26 June 1998

Abstract

Transition probabilities of lines related to odd terms based on the lowest (5D) 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 [FORMULA] 0.06, is the average of the two abundance values proposed in recent literature.

Key words: atomic data – Sun: abundances

* The full Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr/pub/cats/J/A+A/340/300 (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/340/300.

Send offprint requests to: A.J.J. Raassen

© European Southern Observatory (ESO) 1998

Online publication: November 3, 1998

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