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The Colour Magnitude Diagram of a Second Field in the SMC Halo

Published online by Cambridge University Press:  04 August 2017

M.R.S. Hawkins  and
M.T. Brück
M.R.S. Hawkins
Affiliation:
Royal Observatory, Edinburgh EH9 3HJ, U.K.
M.T. Brück
Affiliation:
Royal Observatory, Edinburgh EH9 3HJ, U.K.

Abstract

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A colour magnitude diagram of a field in the south-west periphery of the SMC reveals a population similar to that obtained earlier in another field, with an age of 3 × 109 years. The present field is from the SMC centre, more than a degree more distant than the first one. The similarity in stellar content between the two emphasises the widespread nature of this population.

Type
Evolution
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 101 - 102
Copyright
Copyright © Reidel 1984 

References

Hawkins, M.R.S. and Brück, M.T.: 1982, Mon. Not. R. astr. Soc. 198, 935 CrossRefGoogle Scholar