Broad Iron Lines in AGN and X-Ray Binaries     

A. C. Fabian 《Astrophysics and Space Science》2005,300(1-3):97-105

Several AGN and black hole X-ray binaries show a clear very broad iron line, which is strong evidence that the black holes are rapidly spinning. Detailed 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 carries the imprint of strong gravity at a few gravitational radii. The strong gravitational light bending in these regions then explains the power-law variability as due to changes in height of the primary X-ray source above the disc. The reflection component, in particular its variability and the profile of the iron line, enables us to study the innermost regions around an accreting, spinning, black hole.  相似文献   

RBS 1032: a dwarf-nucleated spheroidal galaxy with an intermediate-mass black hole hosted in a globular cluster     

Kajal K. Ghosh  Valera Suleymanov  Ilfan Bikmaev  Slava Shimansky  Nail Sakhibullin 《Monthly notices of the Royal Astronomical Society》2006,371(4):1587-1593

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Black hole spin in GRS 1915+105   总被引：2，自引：0，他引：2  

Matthew Middleton  Chris Done  Marek Gierli&#;ski  Shane W. Davis 《Monthly notices of the Royal Astronomical Society》2006,373(3):1004-1012

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Neutrino radiation from a collapsing galactic nucleus     

V. I. Dokuchaev 《Astronomy Letters》2002,28(8):522-526

We discuss the possible observational manifestation of the formation of massive black holes in galactic nuclei in the form of an intense high-energy neutrino flux. A short-lived (≤10 yr) hidden neutrino source results from the natural dynamicalal evolution of a central star cluster in the galactic nucleus before its gravitational collapse. The central star cluster at the final evolutionary stage consists of degenerate compact stars (neutron stars and stellar-mass black holes) and is embedded in a massive gaseous envelope produced by destructive collisions of normal stars. Multiple fireballs from frequent collisions of neutron stars give rise to a tenuous quasi-stationary cavity in the central part of the massive envelope. The cavity is filled with shock waves on which an effective cosmic-ray acceleration takes place. Allthe accelerated particles, except the secondary high-energy neutrinos, are absorbed in the dense envelope. The neutrino signal that carries information on the dynamicals of the collapsing galactic nucleus can be recorded by a neutrino detector with an effective area S∼1 km².  相似文献   

On the deep minimum state in the Seyfert galaxy MCG−6-30-15     

Christopher S. Reynolds  Jörn Wilms  Mitchell C. Begelman  Rüdiger Staubert  Eckhard Kendziorra 《Monthly notices of the Royal Astronomical Society》2004,349(4):1153-1166

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On the X-ray spectra of luminous, inhomogeneous accretion flows   总被引：1，自引：0，他引：1  

A. Merloni  J. Malzac  A. C. Fabian  R. R. Ross 《Monthly notices of the Royal Astronomical Society》2006,370(4):1699-1712

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Exploring the Jet/Accretion Flow Relationship in low Disk Luminosity Sources     

Sera Markoff 《Astrophysics and Space Science》2005,300(1-3):189-195

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The star-forming environment of an ultraluminous X-ray source in NGC 4559: an optical study     

Roberto Soria  Mark Cropper  Manfred Pakull  Richard Mushotzky  Kinwah Wu 《Monthly notices of the Royal Astronomical Society》2005,356(1):12-28

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Energy-dependent variability from accretion flows     

Andrzej A. Zdziarski 《Monthly notices of the Royal Astronomical Society》2005,360(3):816-824

We develop a formalism to calculate energy-dependent fractional variability (rms) in accretion flows. We consider rms spectra resulting from radial dependences of the level of local variability (as expected from the propagation of disturbances in accretion flows) assuming the constant shape of the spectrum emitted at a given radius. We consider the cases when the variability of the flow is either coherent or incoherent between different radial zones. As an example of local emission, we consider blackbody, Wien and thermal Comptonization spectra. In addition to numerical results, we present a number of analytical formulae for the resulting rms. We also find an analytical formula for the disc Wien spectrum, which we find to be a very good approximation to the disc blackbody. We compare our results to the rms spectrum observed in an ultrasoft state of GRS 1915+105.  相似文献   

Equilibria of a self-gravitating, rotating disc around a magnetized compact object     

J. Ghanbari  S. Abbassi 《Monthly notices of the Royal Astronomical Society》2004,350(4):1437-1444

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