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Published online by Cambridge University Press: 02 March 2005
A short review on abundance determinations of A and F dwarfs in the Hyades is presented. The spectroscopy was carried out with AURELIE, a monorder spectrograph at the Observatoire de Haute Provence (France) at a resolving power close to 40000 with Signal-to-Noise ratios varying from 100 to 300. Abundances of 11 chemical elements have been derived by using Takeda's (1995) procedure.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html