A New Model for the Hard Time Lags in Black Hole X-Ray Binaries
arXiv:astro-ph/9810064 · doi:10.1086/311833
Abstract
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.
10 pages, including 2 figures; uses epsf.sty, rotate.sty; accepted for ApJ Letters
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- The properties of cross-correlation and spectra of the low-mass X-ray binary 4U 1608-52
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- X-ray energy and power spectra of Seyfert 1 and Narrow Line Seyfert 1 galaxies: comparison to Black Hole Binaries