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

難理解

The Camera Object and Flash Video,eak AGN found in the LINER M81 and higher luminosity Seyfert galaxies. This supports the notion of a continuous sequence of X-ray properties from the Galactic Centre through LINER galaxies to Seyferts, Likely determined by the amount of material available for accretion in the central regions.

烤架

The future of flash in the mobile worldxies. 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.

我說不重要

反感

dominant

鴕鳥

On the relationship between the jets from X-ray binaries and AGN,ack holes of different masses and accretion rates. The regression coefficients of this relation contain information about the nature of the X-ray emission mechanism driving the correlation. We argue that X-ray synchrotron emission from the base of the jets is unlikely to be the dominant contribution to the X-ray spectrum in most of the sources.

CRAB

A transition in the accretion properties of AGN,diative inefficient accretion flows. The (so far) qualitative analogy with the behavior of XRB provides an interesting perspective to find a unique framework for the accretion and jet production in accreting black hole systems.

Minuet

A fundamental plane of black hole activity: Pushing forward the unification scheme,s between the radio (..) and the X-ray (..) luminosity and the black hole mass (.). We find that the radio luminosity is correlated with . and .., at a highly significant level. We show how this result can be used to extend the standard unification by orientation scheme to encompass unification by mass and accretion rate.

陶醉

土坯

Rapid X-ray variability of Seyfert 1 Galaxies,xies. 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.