Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-22T19:40:40.924Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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 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