Hostname: page-component-6bf8c574d5-n2sc8 Total loading time: 0 Render date: 2025-03-09T16:06:31.194Z Has data issue: false hasContentIssue false
  • English
  • Français

A New Look at the Am Stars

Published online by Cambridge University Press:  19 July 2016

C. Burkhart ,
M. F. Coupry  and
C. van't Veer
C. Burkhart
Affiliation:
Observatoire de Lyon, 69230 St Genis-Laval, France
M. F. Coupry
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 75014 Paris, France
C. van't Veer
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 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.

High resolution, high signal-to-noise observations are required for a better understanding of the Am stars and related topics. Two examples are shown : the relationship between lithium content and temperature in the Am stars of the Hyades cluster and the observational problem induced by multiple spectroscopic binarity frequent among the Am stars.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 401 - 406
Copyright
Copyright © Kluwer 1988 

References

Boesgaard, A.M.: 1987, to be published in the Ap.J. Google Scholar
Boesgaard, A.M., Tripicco, M.: 1986, Ap.J. 302, L49 CrossRefGoogle Scholar
Cayrel, R., Cayrel de Strobel, G., Campbell, B., Däppen, W.: 1984, Ap.J. 283, 205 Google Scholar
Fekel, F.C.: 1980, Publ. A .S.P. 92, 785 Google Scholar
Kurucz, R. L.: 1979, Ap.J. Suppl. 40, 1 Google Scholar