Titlebook: From X-ray Binaries to Quasars: Black Holes on All Mass Scales; T. J. Maccarone,R. P. Fender,L. C. Ho Book 2005 Springer Science+Business

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Broad iron lines in AGN and X-ray binaries,led analysis of these objects shows that the emission line is not significantly affected by absorption and that the source variability is principally due to variation in amplitude of a power-law. Underlying this is a much less variable, relativistically-smeared, reflection-dominated, component which

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一個(gè)攪動(dòng)不安

Rapid X-ray variability of Seyfert 1 Galaxies,e powered by a supermassive black hole fed from an accretion disc. However, since . there has been little opportunity to advance our understanding of the most rapid X-ray variability. Observations with . have changed this..We discuss some recent results obtained from . observations of Seyfert 1 gala

Ceremony

Epicyclic frequencies derived from the effective potential: Simple and practical formulae, spacetimes. Such spacetimes include as special cases analytically known black hole Kerr and Schwarzschild spacetimes, as well as the analytic Hartle-Thorne spacetime and all numerically constructed spacetimes relevant for rotating neutron stars. Our derivation follows directly from energy and angul

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X-ray periodicity in AGN,ed from long EUVE light curves of moderate-luminosity Seyfert galaxies; the fourth was discovered in Chandra data from the low-luminosity Seyfert 1 galaxy NGC 4395. When compared with Cyg X-1, I find that the period is related to the luminosity as . ∝ .. rather than the expected one-to-one relations

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buoyant

Concerto

X-ray and radio monitoring of GX 339-4 and CYG X-1,y agrees with the IR flux level. Corbel and Fender [2002, . 573, L35—L39] later showed that the typical hard state radio power-law extrapolated forward in energy meets the backward extrapolated X-ray power-law at an IR spectral break, which was explicitly observed twice in GX 339-4. This has been ci

Scleroderma

Baffle

Springer Science+Business Media B.V. 2005