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

被引：0

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

关键词：

Color;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Journal article (JA)

引用

页码：165 / 176

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