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000001855 037__ $$aASTROimport-12
000001855 100__ $$aGrevesse, N.
000001855 245__ $$aThe solar abundance of iron and the photospheric model
000001855 260__ $$c1999
000001855 520__ $$aNumerous papers on the solar photospheric abundance of iron have recently been published leading to a longstanding debate concerning rather different results obtained from the analyses of Fe i lines and, to a lesser extent, of Fe ii lines. Based on a set of 65 solar Fe i lines, with accurate transition probabilities as well as new accurate damping constants, we construct a new empirical photospheric model. We succeed to reconcile abundance results obtained from low and high excitation Fe i lines as well as from Fe ii lines and derive a solar photospheric abundance of iron, A_Fe = 7.50 +/- 0.05, which perfectly agrees with the meteoritic value. A detailed version of Table~2 is available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or at the ORB via anonymous ftp to ftpserver.oma.be/pub/astro/jacques. 
000001855 700__ $$a Sauval, A. J.
000001855 773__ $$c348-354$$pAstronomy and Astrophysics$$v347$$y1999
000001855 85642 $$ahttp://esoads.eso.org/abs/1999A%26A...347..348G
000001855 905__ $$apublished in
000001855 980__ $$aREFERD