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Astron. Astrophys. 359, 743-754 (2000)
Acknowledgements
It is a pleasure to thank Paul Barklem, Sveneric Johansson and Jim O'Mara for helpful discussions and for providing unpublished line data in terms of line broadening and laboratory wavelengths. Discussions with Natalia Shchukina regarding departures from LTE for Fe are much appreciated, as are the constructive suggestions by an anonymous referee. Extensive use have been made of the VALD database (Kupka et al. 1999), which is gratefully acknowledged.
© European Southern Observatory (ESO) 2000
Online publication: July 7, 2000
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