X-ray Variability of AGN and the Flare Model - IN2P3 - Institut national de physique nucléaire et de physique des particules Access content directly
Conference Papers Year : 2007

X-ray Variability of AGN and the Flare Model

R. W. Goosmann
  • Function : Author
B. Czerny
  • Function : Author
A.-M. Dumont
  • Function : Author
M. Mouchet
  • Function : Author
A. Rózanska
  • Function : Author

Abstract

Short-term variability of X-ray continuum spectra has been reported for several Active Galactic Nuclei. Significant X-ray flux variations are observed within time scales down to 10^3-10^5 seconds. We discuss short variability time scales in the frame of the X-ray flare model, which assumes the release of a large hard X-ray flux above a small portion of the accretion disk. The resulting observed X-ray spectrum is composed of the primary radiation and of a reprocessed Compton reflection component that we model with numerical radiative transfer simulations. The incident hard X-rays of the flare will heat up the atmosphere of the accretion disk and hence induce thermal expansion. Eventually, the flare source will be surrounded by an optically-thick medium, which should modify the observed spectra.
No file

Dates and versions

in2p3-00184659 , version 1 (31-10-2007)

Identifiers

Cite

R. W. Goosmann, B. Czerny, A.-M. Dumont, M. Mouchet, A. Rózanska. X-ray Variability of AGN and the Flare Model. AGN Variability from X-Rays to Radio Waves, Jun 2004, Crimée, Ukraine. pp.277. ⟨in2p3-00184659⟩
11 View
0 Download

Share

Gmail Mastodon Facebook X LinkedIn More