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The variable star population of NGC 1866

Published online by Cambridge University Press:  19 July 2016

Douglas L. Welch ,
Patrick Côté ,
Mario Mateo  and
Barry F. Madore
Douglas L. Welch
Affiliation:
Dept. of Physics, McMaster University, Hamilton, Ontario L8S 4M1, Canada
Patrick Côté
Affiliation:
Dept. of Physics, McMaster University, Hamilton, Ontario L8S 4M1, Canada
Mario Mateo
Affiliation:
Observatories of the Carnegie Institution of Washington, 813 Santa Barbara St, Pasadena, CA 91101, USA
Barry F. Madore
Affiliation:
Infrared Processing & Analysis Center, Jet Propulsion Laboratory, M/S 100-22, California Institute of Technology, Pasadena, CA 91125, USA

Abstract

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We report the results of an extensive photometric and radial velocity study of the variable stars in the Large Magellanic Cloud (LMC) cluster NGC 1866. We find:

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 384 - 385
Copyright
Copyright © Kluwer 1991 

References

Freeman, K.C., Illingworth, G., Oemler, A. (1983), Astrophys. J. 272, 488.CrossRefGoogle Scholar
Mateo, M., Schechter, P. (1989), Proceedings of the First ESO Data Analysis Workshop , in press.Google Scholar
Stetson, P.B. (1987), Publ. Astron. soc. Pac. 99, 191.CrossRefGoogle Scholar
Storm, J., Andersen, J., Blecha, A., Walker, M.F. (1988), Astron. Astrophys. 190, L18.Google Scholar
Walker, A.R. (1987), M.N.R.A.S. 225, 627.CrossRefGoogle Scholar