Strong soft X-ray emission and high accretion rates in Seyfert galaxies

被引：0
|
作者：
Szuszkiewicz, E [1 ]
机构：
[1] Univ Leicester, Dept Phys & Astron, Astron Grp, Leicester LE1 7RH, Leics, England
来源：
ACCRETION PHENOMENA AND RELATED OUTFLOWS: IAU COLLOQUIUM 163 | 1997年 / 121卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Slim accretion disk models with high accretion rates provide a natural explanation for the strong soft X-ray emission observed in several narrow-line Seyfert 1 galaxies.
引用
收藏
页码：812 / 813
页数：2
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