Kottamia 74-inch telescope discovery of the new eclipsing binary 2MASS J20004638+0547475.: First CCD photometry and light curve analysis

被引:9
作者
Darwish, M. S. [1 ,2 ]
Shokry, A. [1 ,2 ]
Saad, S. M. [1 ,2 ]
El-Sadek, M. A. [1 ,2 ]
Essam, A. [1 ]
Ismail, M. [1 ,2 ]
机构
[1] Natl Res Inst Astron & Geophys, Dept Astron, Cairo, Egypt
[2] Kottamia Ctr Sci Excellence Astron & Space Sci KC, STDF, ASRT, Cairo, Egypt
关键词
2mass j20004638+0547475; Evolution; W Uma; Eclipsing binary and mass transfer; STARS;
D O I
10.1016/j.newast.2016.11.009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A CCD photometric study is presented for the eclipsing binary system 2MASSJ20004638 + 0547475. Observations of the system were obtained in the V, R and I colours with the 2Kx2K CCD attached to 1.88 m Kottamia Optical Telescope. New times of light minimum and new ephemeris were obtained. The V, R and I light curves were analyzed using the PHOEBE 0.31 program to determine geometrical and physical parameters of the system. The results show that 2MASS J20004638 + 0547475, is A-Type WUMa and is an overcontact binary with high fill-out factor =69%. The current evolutionary status of the system indicates that the primary component lies very close to the main sequence while the secondary is evolved. The asymmetric maxima were studied and a modeling of the hot spot parameters is given. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:35 / 38
页数:4
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