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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

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