A New Model for the Hard Time Lags in Black Hole X-Ray Binaries

Details A New Model for the Hard Time Lags in Black Hole X-Ray Binaries A New Model for the Hard Time Lags in Black Hole X-Ray Binaries

1998-10-05

arxiv.org/abs/astro-ph/9810064v2

Astronomy and Astrophysics

Astrophysics

10 pages, including 2 figures; uses epsf.sty, rotate.sty; accepted for ApJ Letters

Scientific paper

10.1086/311833

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.

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