PHOTOMETRY RESULT OF AN ECLIPSING BINARY STAR V798Her IN THE GLOBULAR CLUSTER NGC 6341

被引：0
|
作者：
Anees, Khola [1 ]
Goderya, Shaukat [2 ]
机构：
[1] Inst Space Technol, Islamabad, Pakistan
[2] Tarleton State Univ, Stephenville, TX USA
来源：
2019 SIXTH INTERNATIONAL CONFERENCE ON AEROSPACE SCIENCE AND ENGINEERING (ICASE) | 2019年
关键词：
CCD Photometry; Eclipsing Binary Stars;
D O I：
暂无
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
We present the photometric study of an eclipsing binary star V798Her in the globular cluster NGC 6341. The observations were obtained in Johnson's B, V & R filters using 0.8m Tarleton telescope and a CCD photometer. The observed light curves after determination of light elements show that V798Her is a W UMa contact binary system with a period of 0.2951110 days. This binary system will be further analyzed using Wilson Devinney model 2015 version.
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页码：154 / 156
页数：3
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