Hostname: page-component-6bf8c574d5-t27h7 Total loading time: 0 Render date: 2025-02-21T20:11:49.379Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Boesgaard, A.M. 1987, ApJ 321, 967 Google Scholar
Burkhart, C., Coupry, M.F. 1989, A&A 220, 197 Google Scholar
Michaud, G. 1992, The Atmospheres of Early-Type Stars, in Lecture Notes in Physics 401, Eds. Heber, U. and Jeffery, C.S., p. 189 Google Scholar
Richer, J. 1992, Thèse de doctorat, Univ. de Montréal, in preparationGoogle Scholar
Schwan, H. 1991, A&A 243, 386 Google Scholar
Vauclair, S. 1991, Evolution of Stars: The Photospheric Abundance Connection, IAU Symposium 145, Eds. Michaud, G. and Tutukov, A.), p. 327 Google Scholar