... BD +17 4708[*]
Tables 2, 3 and Appendix are only available in electronic form at http://www.aanda.org 
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... Redfield[*]
Hubble Fellow. 
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...)[*]
Throughout this paper, we use the standard definitions $[X/Y]=\log(N_X/N_Y)-\log(N_X/N_Y)_\odot$ and $A_{X}=\log(N_X/N_{\rm H})+12$, where NX is the number density of the element X. The surface gravity g in $\log g$ is given in cgs units. 
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... R. L. Kurucz[*]
Up-to-date models are available at http://kurucz.harvard.edu. The characteristics of the models are explained in Kurucz (1970, 1979). 
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... a MARCS model[*]
Downloaded from http://marcs.astro.uu.se 
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...)[*]
By "spectroscopic'' here we refer to  $T_{{\rm eff}}$ obtained from the excitation and/or ionization balance of iron lines. 
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... IRAF[*]
IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation - http://iraf.noao.edu 
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...1973)[*]
http://verdi.as.utexas.edu/moog.html 
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... Database[*]
http://physics.nist.gov/PhysRefData/ASD/lines_form.html 
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...1995)[*]
http://nova.astro.umd.edu 
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... abundance[*]
Our line list and adopted atomic data result in $A_{{\rm Fe},\odot}=7.51$ $\pm$ 0.08, with no significant difference between the Fe I and Fe II abundances, although not all the lines could be used in the solar spectrum due to saturation. Details will be given in Ramírez et al. (2006). 
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... 0.09[*]
Unless otherwise noted, all the error bars for the abundances are 1-$\sigma $ errors. 
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...2004b)[*]
Allende Prieto et al. used both 1D and 3D model atmospheres in their study. We remind the reader that our work is restricted to 1D Kurucz models. 
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Copyright ESO 2006