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arXiv · astro-ph/0412695

Rapid X-ray Variability of Seyfert 1 Galaxies

S. Vaughan·A. C. Fabian·K. Iwasawa
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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.

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S. Vaughan, A. C. Fabian, K. Iwasawa. 2004-12-30. Rapid X-ray Variability of Seyfert 1 Galaxies. https://doi.org/10.1007/s10509-005-1211-x

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