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Carbon Stars in the SMC

Published online by Cambridge University Press:  26 July 2016

D.H. Morgan  and
D. Hatzidimitriou
D.H. Morgan
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, U.K.
D. Hatzidimitriou
Affiliation:
University of Crete and Institute of Electronic Structure and Laser, P.O. Box 1527, GR 711-10 Heraklion, Crete, Greece

Abstract

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More than 1000 new carbon stars have been identified in a ∼200 deg2 area of the SMC during a survey of UK Schmidt Telescope objective-prism plates. Their spatial distribution is like that of the red horizontal branch stars.

Type
Part Ten: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 513 - 515
Copyright
Copyright © Kluwer 1994 

References

Azzopardi, M., 1993. In ‘New aspects of Magellanic Cloud Research’, eds. Baschek, B., Klare, G. and Lequeux, J., Proc. Heidelberg, Germany, p. 86.Google Scholar
Gardiner, L.T. and Hatzidimitriou, D., 1992. Mon. Not. R. astron. Soc., 257, 195. (GH92).Google Scholar
Rebeirot, E., Azzopardi, M. and Westerlund, B.E., 1993. Astron. Astrophys. Suppl., 97, 603. (RAW93).Google Scholar