The variability mechanism of Seyfert galaxy NGC 4151

被引：4
|
作者：
Fan, JH [1 ]
Su, CY
Lin, RG
机构：
[1] Guangzhou Univ, Ctr Astrophys, Guangzhou 510405, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
[3] Guangdong Ind Univ, Dept Phys, Guangzhou 510643, Peoples R China
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2002年 / 54卷 / 02期
关键词：
accretion; accretion disks; galaxies : individual (NGC 415 1); galaxies : Seyfert; instabilities;
D O I：
10.1093/pasj/54.2.175
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Based on compilation by Fan and Su (1998, AAA 70.158.417), the variability property is discussed for the Seyfert galaxy NGC 415 1 using the structure function, V(tau)(1/2) similar to tau(k). The derived k is 0.35 +/- 0.03, suggesting that the disk-instability favors the star-burst model as an explanation for the mechanism of the variability in this source.
引用
收藏
页码：175 / 178
页数：4
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