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- W2949602016 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." @default.
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- W2949602016 date "2005-11-01" @default.
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- W2949602016 title "Rapid X-Ray Variability of Seyfert 1 Galaxies" @default.
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- W2949602016 doi "https://doi.org/10.1007/s10509-005-1211-x" @default.
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