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The abundances of A/F and Am/Fm stars in open clusters

Published online by Cambridge University Press:  02 March 2005

Richard Monier  and
Olivier Richard
Richard Monier
Affiliation:
GRAAL, Universite Montpellier II, Place E. Bataillon, 34095 Montpellier, France email: Richard.Monier@graal.univ-montp2.fr, Olivier.Richard@graal.univ-montp2.fr
Olivier Richard
Affiliation:
GRAAL, Universite Montpellier II, Place E. Bataillon, 34095 Montpellier, France email: Richard.Monier@graal.univ-montp2.fr, Olivier.Richard@graal.univ-montp2.fr
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Abstract

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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

Keywords

Stars: abundancesstars: chemically peculiarGalaxy:open clusters and associations: individual: Hyadesdiffusion
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 528 - 529
Copyright
© 2004 International Astronomical Union