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Time-Series CCD Photometry of Northern Open Clusters Using the BOAO 1.8-m Telescope: III. NGC 2301

Published online by Cambridge University Press:  12 April 2016

S.-L. Kim ,
B.-G. Park ,
M.-Y. Chun ,
H. Sung ,
Y.-B. Jeon ,
I.-S. Yuk ,
H. B. Ann ,
S. H. Lee  and
M. G. Lee
S.-L. Kim
Affiliation:
Korea Astronomy Observatory, Korea
B.-G. Park
Affiliation:
Korea Astronomy Observatory, Korea
M.-Y. Chun
Affiliation:
Korea Astronomy Observatory, Korea
H. Sung
Affiliation:
Korea Astronomy Observatory, Korea
Y.-B. Jeon
Affiliation:
Korea Astronomy Observatory, Korea
I.-S. Yuk
Affiliation:
Korea Astronomy Observatory, Korea
H. B. Ann
Affiliation:
Department of Earth Science, Pusan National University, Korea
S. H. Lee
Affiliation:
Department of Earth Science, Pusan National University, Korea
M. G. Lee
Affiliation:
Department of Astronomy, Seoul National University, Korea

Abstract

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A time-series CCD photometric survey of variable stars in open clusters has been in progress using 1.8-m telescope at the Bohyunsan Optical Astronomy Observatory (BOAO) in Korea. We present preliminary results of time series photometry for the intermediate-age open cluster NGC 2301.

Type
Part 6. Variables Close to the Main Sequence
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 457 - 458
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Ann, H.B., Lee, M.G., Chun, M.-Y., Kim, S.-L., et al. 1999, JKAS, 32, 7 Google Scholar
Gilliland, R.L. & Brown, T.M. 1988, PASP, 100, 754 Google Scholar