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New results on the structure and stellar content of the outer regions of the SMC

Published online by Cambridge University Press:  19 July 2016

L. T. Gardiner  and
M.R.S. Hawkins
L. T. Gardiner
Affiliation:
Department of Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United Kingdom
M.R.S. Hawkins
Affiliation:
Royal Observatory, Edinburgh EH9 3HJ, United Kingdon

Abstract

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Surface distribution contour maps of the HB/clump population and the < 1 Gyr main sequence population for the outer regions of the Small Magellanic Cloud (SMC) are presented. Aspects of the stellar population synthesis, large-scale structure and evolutionary history of the SMC halo are discussed.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 51 - 52
Copyright
Copyright © Kluwer 1991 

References

De Vaucouleurs, G., Freeman, K.C. (1972), Vistas Astr. 14, 163.Google Scholar
Hatzidimitriou, D. (1989), Ph.D thesis.Google Scholar
Hatzidimitriou, D., Hawkins, M.R.S., Gyldenkerne, K. (1989), MNRAS 241, 645.Google Scholar
Mathewson, D.S., Ford, V.L. (1984), IAU Symp. 108 Structure and Evolution of the Magellanic Clouds , van den Bergh, S. and de Boer, K.S. (eds.) (Reidel: Dordrecht) p. 125.CrossRefGoogle Scholar
Murai, T., Fujimoto, M. (1986), Astrophys. Sp. Sci. 119, 169.Google Scholar