Rapid X-ray Variability of Seyfert 1 Galaxies
Abstract
The rapid and seemingly random fluctuations in X-ray luminosity of Seyfert galaxies provided early support for the standard model in which Seyferts are powered by a supermassive black hole fed from an accretion disc. However, since EXOSAT there has been little opportunity to advance our understanding of the most rapid X-ray variability. Observations with XMM-Newton have changed this. We discuss some recent results obtained from XMM-Newton observations of Seyfert 1 galaxies. Particular attention will be given to the remarkable similarity found between the timing properties of Seyferts and black hole X-ray binaries, including the power spectrum and the cross spectrum (time delays and coherence), and their implications for the physical processes at work in Seyferts.
Cite
@article{arxiv.astro-ph/0412695,
title = {Rapid X-ray Variability of Seyfert 1 Galaxies},
author = {S. Vaughan and A. C. Fabian and K. Iwasawa},
journal= {arXiv preprint arXiv:astro-ph/0412695},
year = {2009}
}
Comments
To appear in From X-ray Binaries to Quasars: Black Hole Accretion on All Mass Scales, ed. T. J. Maccarone, R. P. Fender, and L. C. Ho (Dordrecht: Kluwer)