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Two more Magellanic Cloud CM diagrams

Published online by Cambridge University Press:  19 July 2016

J.R. Mould ,
J. B. Jensen ,
G.S. Da Costa ,
J. Kristian  and
J.M. Nemec
J.R. Mould
Affiliation:
Palomar Observatory, California Inst. of Tech., Pasadena, Calif. 91125, USA
J. B. Jensen
Affiliation:
Palomar Observatory, California Inst. of Tech., Pasadena, Calif. 91125, USA
G.S. Da Costa
Affiliation:
Anglo Australian Observatory, Epping, NSW, Australia
J. Kristian
Affiliation:
Observatories of the Carnegie Institution of Washington, Pasadena, Calif. 91101, USA
J.M. Nemec
Affiliation:
University of British Columbia, Vancouver, BC V6T 1W5, Canada

Abstract

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Lindsay 11 and NGC 1806 are globular clusters in the Small and Large Magellanic Clouds (SMC and LMC) respectively. Both clusters have extended asymptotic giant branches with carbon stars at the tip. Colour-magnitude diagrams are fitted with appropriate isochrones which indicate that both clusters belong to the abundant population of intermediate age in the Magellanic Clouds.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 357 - 359
Copyright
Copyright © Kluwer 1991 

References

Da Costa, G., Mould, J., Crawford, M. (1985), Astrophys. J. 297, 582.Google Scholar
Frogel, J., Mould, J., Blanco, V. (1990), Astrophys. J. 352, 96.Google Scholar
Iben, I., Renzini, A. (1983), Ann. Rev. Astron. Astrophys. 21, 271.Google Scholar
Vanden Berg, D. (1985), Astrophys. J. Suppl. 58, 711.Google Scholar