Photometric and spectroscopic study of the eclipsing binary GSC 4288 0186

被引：0
|
作者：
Bakis, V. [1 ,2 ]
Bakis, H. [1 ,2 ]
Budding, E. [1 ,2 ]
Demircan, O. [1 ]
Zejda, M. [3 ]
机构：
[1] Canakkale Univ, Dept Phys, TR-17020 Canakkale, Turkey
[2] Carter Observ, Wellington, New Zealand
[3] Masaryk Univ, Inst Theoret Phys & Astrophys, CZ-61137 Brno, Czech Republic
来源：
SOLAR AND STELLAR PHYSICS THROUGH ECLIPSES | 2007年 / 370卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
First complete BVRI light curves and radial velocity measurements of the recently discovered eclipsing binary GSC 4288 0186 are presented. Analyses of the light curves, together with spectroscopic data show that the system is a double-lined detached binary with an eccentric orbit. We determined the preliminary values of the absolute elements of this eclipsing binary and presented here.
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页码：213 / +
页数：2
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