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Metal abundances of Magellanic Cloud clusters

Published online by Cambridge University Press:  07 August 2017

D. Geisler ,
N. Suntzeff ,
M. Mateo  and
J. Graham
D. Geisler
Affiliation:
Cerro Tololo Inter-American Observatory Casilla 603, La Serena, Chile
N. Suntzeff
Affiliation:
Cerro Tololo Inter-American Observatory Casilla 603, La Serena, Chile
M. Mateo
Affiliation:
Observatories of The Carnegie Institution of Washington 813 Santa Barbara Street, Pasadena, CA 91101
J. Graham
Affiliation:
Observatories of The Carnegie Institution of Washington 813 Santa Barbara Street, Pasadena, CA 91101

Abstract

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High signal—to-noise ratio, medium resolution spectra have been obtained for ~8 giants in each of 18 LMC clusters with the CTIO 4-m multifiber ARGUS spectrograph. In addition, Washington CCD photometry has been obtained for ~50 SMC and LMC clusters with the CTIO 4-m and 1.5-m from which abundances can be obtained for ~25 giants per cluster. The derivation of metal abundances from these data will be discussed and some preliminary results presented.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 422
Copyright
Copyright © Kluwer