On the difference between radio quiet and radio loud AGN

被引：0
|
作者：
Marziani, P [1 ]
Calvani, M [1 ]
Sulentic, JW [1 ]
机构：
[1] Osservatorio Astron Padova, I-35122 Padua, Italy
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：
A systematic difference in alignment between the central black hole spin and the angular momentum of the accreting gas may help to explain several differences found in the optical and UV HST spectra of radio loud and radio quiet AGN.
引用
收藏
页码：761 / 762
页数：2
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