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High Signal to Noise Analysis of the Chemical Composition of Stars in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

M. Spite ,
F. Spite  and
P. François
M. Spite
Affiliation:
Observatoire de Paris-Meudon 92195 Meudon Cedex (France)
F. Spite
Affiliation:
Observatoire de Paris-Meudon 92195 Meudon Cedex (France)
P. François
Affiliation:
E.S.O., Karl Schwarzschild str. 2 8046 Garching bei München (F. R. G.)

Abstract

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A few high S/N spectra of F-G supergiants in the field of the Magellanic Clouds, and a spectrum of a star in the in the young SMC cluster NGC330 have been obtained at the échelle spectrograph of the 3.6m telescope of ESO (CASPEC). Preliminary results of the analysis of these stars and their consequences in the evolution of the clouds are presented here.

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. 551 - 554
Copyright
Copyright © Kluwer 1988 

References

Bica, E., Dottori, H., Pastoriza, M.: 1986, Astron. Astrophys. 156, 261 Google Scholar
Cayrel, R.: 1986, Astron. Astrophys. 168, 81 Google Scholar
Dufour, R.J.: 1983, in IAU symposium 108 p.353 (Van den Bergh, S. and de Boer, K., eds.) Richtler, T., Nelles, B.: Astron. Astrophys. 119, 75 Google Scholar
Spite, M., Cayrel, R., François, P., Richtler, T., Spite, F.: 1986, Astron. Astrophys. 168, 197 Google Scholar
Stryker, L.L., Da Costa, G.S., Mould, J.R.: 1986, Astrophys. J. 298, 544 CrossRefGoogle Scholar