PHOTOMETRIC STUDY OF THE SEYFERT GALAXY NGC 4151

被引：0
|
作者：
Shomshekova, S. A. [1 ]
Kusakin, A. V. [1 ]
Reva, I. V. [1 ]
机构：
[1] VG Fesenkov Astrophys Inst, Alma Ata 050020, Kamenskoye Plat, Kazakhstan
来源：
BALTIC ASTRONOMY | 2016年 / 25卷 / 03期
关键词：
galaxies: Seyfert; galaxies: individual (NGC 4151); galaxies: photometry; NGC-4151; STARS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The results of CCD photometry in the Johnson-Morgan BVR system for the Seyfert galaxy NGC 4151 are reported. The observations were carried out from November 15, 2013 to May 13, 2016 with the 1-m telescope of Tien-Shan Astronomical Observatory of the Fesenkov Astrophysical Institute. An analysis of the light curve of NGC 4151 shows that over the time interval considered the brightness of the object varied synchronously in the three filters with the following amplitudes: Delta B = 0.68 mag, Delta V = 1.09 mag, and Delta R = 1.81 mag.
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收藏
页码：275 / 279
页数：5
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