A new model for the hard time lags in black hole X-ray binaries

被引：53

作者：

Böttcher, M ^{[1
]}

Liang, EP ^{[1
]}

机构：

[1] Rice Univ, Dept Space Phys & Astron, Houston, TX 77005 USA

来源：

ASTROPHYSICAL JOURNAL | 1999年 / 511卷 / 01期

基金：

美国国家航空航天局;

关键词：

accretion; accretion disks; black hole physics; radiation mechanisms : thermal; radiative transfer; X-rays : stars;

D O I：

10.1086/311833

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The time-dependent Comptonized output of a cool soft X-ray source drifting inward through an inhomogeneous hot inner disk or corona is numerically simulated. We propose that this scenario can explain from first principles the observed trends in the hard time lags and power spectra of the rapid aperiodic variability of the X-ray emission of Galactic black hole candidates.

引用

页码：L37 / L40

页数：4

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