Close binary and other variable stars in the solar-age galactic open cluster M67

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作者：
Yakut, K. [1 ,2 ,3 ]
Zima, W. [1 ]
Kalomeni, B. [2 ,4 ]
VanWinckel, H. [1 ]
Waelkens, C. [1 ]
De Cat, P. [1 ,5 ]
Bauwens, E. [1 ]
Vučković, M. [1 ]
Saesen, S. [1 ]
Le Guillou, L. [1 ,6 ]
Parmaksizoǧlu, M. [7 ]
Uluç, K. [7 ]
Khamitov, I. [7 ]
Raskin, G. [1 ]
Aerts, C. [1 ,8 ]
机构：
[1] Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
[2] University of Cambridge, Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, United Kingdom
[3] University of Ege, Department of Astronomy and Space Sciences, 35100 Izmir, Turkey
[4] Izmir Institute of Technology, Department of Physics, 35430 Izmir, Turkey
[5] Royal Observatory of Belgium, Ringlaan 3, 1180 Brussel, Belgium
[6] LPNHE, Université Paris, 75252 Paris Cedex 05, France
[7] TÜBITAK National Observatory, Antalya, Turkey
[8] IMAPP, Radboud Universiteit Nijmegen, PO Box 9010, 6500 GL Nijmegen, Netherlands
来源：
Astronomy and Astrophysics | 2009年 / 503卷 / 01期
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页码：165 / 176
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