ACTIVE GALACTIC NUCLEI .5. X-RAY VARIABILITY AND THE BLACK-HOLE CLUSTER PARADIGM

被引：4

作者：

PACHOLCZYK, AG ^{[1
]}

STOEGER, WR ^{[1
]}

机构：

[1] UNIV ARIZONA,STEWARD OBSERV,VATICAN OBSERV RES GRP,TUCSON,AZ 85721

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 434卷 / 02期

关键词：

BLACK HOLE PHYSICS; GALAXIES; ACTIVE; NUCLEI; SEYFERT; X-RAYS;

D O I：

10.1086/174745

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A random superposition of elementary luminosity bursts of rectangular or triangular shape produces X-ray luminosity flicker curves characterized by features corresponding to those observed in the X-ray-variable Seyfert galaxies and other active galactic nuclei. Such luminosity events could be produced by accretion processes resulting from tidal disruption and consumption of stars by small (approximately 1 M.) black holes, or much more frequently from such holes passing and disrupting accretion disks belonging to large holes in a nuclear cluster.

引用

页码：435 / 445

页数：11

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