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Search for Variable Stars in the Open Cluster NGC 2539

Published online by Cambridge University Press:  12 April 2016

K.J. Choo
Affiliation:
Dept. of Astronomy and Atmospheric Sciences, Kyungpook National Univ., Taegu, 702-701, Korea Korea Astronomy Observatory, Taejon, 305-348, Korea
S.-L. Kim
Affiliation:
Korea Astronomy Observatory, Taejon, 305-348, Korea
T. S. Yoon
Affiliation:
Dept. of Astronomy and Atmospheric Sciences, Kyungpook National Univ., Taegu, 702-701, Korea
M.-Y. Chun
Affiliation:
Korea Astronomy Observatory, Taejon, 305-348, Korea
H. Sung
Affiliation:
Korea Astronomy Observatory, Taejon, 305-348, Korea
B.-G. Park
Affiliation:
Dept. of Astronomy and Atmospheric Sciences, Kyungpook National Univ., Taegu, 702-701, Korea Korea Astronomy Observatory, Taejon, 305-348, Korea
H. B. Ann
Affiliation:
Dept. of Earth Sciences, Pusan National Univ., Pusan, 609-135, Korea
M. G. Lee
Affiliation:
Astronomy Program, SEES, Seoul National Univ., Seoul, 151-741, Korea
Y.-B. Jeon
Affiliation:
Korea Astronomy Observatory, Taejon, 305-348, Korea Astronomy Program, SEES, Seoul National Univ., Seoul, 151-741, Korea
I.-S. Yuk
Affiliation:
Korea Astronomy Observatory, Taejon, 305-348, Korea Astronomy Program, SEES, Seoul National Univ., Seoul, 151-741, Korea

Abstract

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We report on the results of CCD photometric observations of the open cluster NGC 2539. Eight new variable stars have been found in the observed field of this cluster. However, no γ Doradus-type variability was found among the member stars.

Type
V. Variability Study
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

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