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Li in Clusters: A and Am Stars

Published online by Cambridge University Press:  12 April 2016

C. Burkhart  and
M.F. Coupry
C. Burkhart
Affiliation:
Observatoire de Lyon 69561 Saint-Genis-Laval Cedex, France
M.F. Coupry
Affiliation:
Observatoire de Paris 61 Avenue de l’Observatoire, 75014 Paris, France

Abstract

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A and Am stars were observed in open clusters for their Li content. The Li abundance is therefore studied on the hot side of the Li gap along isochrones. It is discussed in relation to evolutionary model atmospheres including particle transport processes.

Type
I. General Properties of CP Stars
Information
International Astronomical Union Colloquium , Volume 138: Peculiar versus Normal Phenomena in A-Type and Related Stars , 1993 , pp. 187 - 191
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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