A CCD photometric study of the W UMa contact binary RZ Comae
被引:8
作者:
Xiang, FY
论文数: 0引用数: 0
h-index: 0
机构:
Xiangtan Univ, Dept Phys, Xiangtan 411105, Hunan, Peoples R ChinaXiangtan Univ, Dept Phys, Xiangtan 411105, Hunan, Peoples R China
Xiang, FY
[1
]
Zhou, YC
论文数: 0引用数: 0
h-index: 0
机构:
Xiangtan Univ, Dept Phys, Xiangtan 411105, Hunan, Peoples R ChinaXiangtan Univ, Dept Phys, Xiangtan 411105, Hunan, Peoples R China
Zhou, YC
[1
]
机构:
[1] Xiangtan Univ, Dept Phys, Xiangtan 411105, Hunan, Peoples R China
来源:
NEW ASTRONOMY
|
2004年
/
9卷
/
04期
基金:
中国国家自然科学基金;
关键词:
binaries : close;
stars : individual : RZ com;
D O I:
10.1016/j.newast.2003.12.001
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
In this paper a B-band light curve of the W UMa contact binary RZ Com is presented. From the observations, five times of light minimum were determined. The light curve was analyzed by means of the latest version of the Wilson-Devinney code. The results suggest that RZ Com is a W-subtype contact with a mass ratio of q = m(2) /m(1) = 2.226. In the new photometric solution, the photospheric temperature of the secondary T-2 = 4842 +/- 8 K. It is slightly lower than the photospheric temperature of the primary T-1. (C) 2003 Elsevier B.V. All rights reserved.