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A Variable Star Survey of the Open Cluster NGC 2126

Published online by Cambridge University Press:  12 April 2016

A. Derekas
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
L.L. Kiss
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
T.R. Bedding
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
A. Gáspár
Affiliation:
Department of Experimental Physics, University of Szeged, Hungary
K. Sárneczky
Affiliation:
Department of Experimental Physics, University of Szeged, Hungary
Gy.M. Szabó
Affiliation:
Department of Experimental Physics, University of Szeged, Hungary
M. Váradi
Affiliation:
Department of Experimental Physics, University of Szeged, Hungary
S. Kaspi
Affiliation:
School of Physics and Astronomy and the Wise Observatory, Tel-Aviv University, Tel-Aviv 69978, Israel
Cs. Kiss
Affiliation:
Konkoly Observatory of the Hungarian Academy of Sciences, P. 0. Box 67, H-1525 Budapest, Hungary

Abstract

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We present the first CCD photometric observations of the northern open cluster NGC 2126. Data were taken on eight nights in 2002 February and December with a total time span of ~57 hours. We have discovered six new variable stars and have estimated the main characteristics of the cluster.

Type
Part 3. Variable stars as tracers of different stellar populations – galactic and globular clusters, LMC/SMC and Local Group galaxies
Copyright
Copyright © Astronomical Society of the Pacific 2004

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