On the variability coherence observed in black hole candidates at different X-ray energies

被引：2

作者：

Abramowicz, MA

Bao, G

Larsson, S

Wiita, PJ

机构：

[1] CHALMERS UNIV TECHNOL,S-41296 GOTHENBURG,SWEDEN

[2] NORDITA,DK-2100 COPENHAGEN,DENMARK

[3] SCUOLA INT SUPER STUDI AVANZATI,LAB INTERDISCIPLINARE,I-34014 TRIESTE,ITALY

[4] INT CTR THEORET PHYS,I-34014 TRIESTE,ITALY

[5] GEORGIA STATE UNIV,DEPT PHYS & ASTRON,ATLANTA,GA 30303

[6] STOCKHOLM OBSERV,S-13336 SALTSJOBADEN,SWEDEN

来源：

ASTROPHYSICAL JOURNAL | 1997年 / 489卷 / 02期

关键词：

accretion; accretion disks; black hole physics; X-rays; general; stars;

D O I：

10.1086/304833

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The bright spot model explains in a natural way the variability coherence observed in black hole candidates at different X-ray energies.

引用

收藏

页码：819 / 821

页数：3

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