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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疏忽

FATAL

Jet-disc coupling in the accreting black hole XTE J1118+480,ting synchrotron radiation in the optical band.We propose a scenario in which the jet and the X-ray corona are fed by the same energy reservoir where large amounts of accretion power are stored before being channelled into either the jet or the high energy radiation. This time-dependent model reprod

Ergots

Awning

A fundamental plane of black hole activity: Pushing forward the unification scheme,X-ray and radio bands. We compile a sample of ～100 active galactic nuclei with measured mass, 5 GHz core emission, and 2–10 keV luminosity, together with eight galactic black holes with a total of ～50 simultaneous observations in the radio and X-ray bands. Using this sample, we study the correlation

字形刻痕

Feature

Liberate

Black hole spin in AGN and GBHCs,ess with which X-ray spectroscopy can be used to probe strong gravity, we summarize how these techniques can constrain black hole spin. In particular, we highlight . studies of the Seyfert galaxy MCG-6-30-15 and the stellarmass black hole GX 339-4. The broad X-ray iron line profile, together with re

Exposition

The Seyfert-liner galaxy NGC 7213: An , observation,on lines from Fe I, Fe . and Fe . and a soft X-ray collisionally ionised thermal plasma with . = 0.18. keV. We find a luminosity of 7 × 10. L., and a lack of soft X-ray excess emission, suggesting a truncated accretion disc. NGC 7213 has intermediate X-ray spectral properties, between those of the w

OGLE

Observational effects of strong gravity,nt horizon. As such, these photons are subject to general relativistic effects such as light-bending, gravitational lensing and redshift, time-dilation, etc. These gravitational effects are well-understood from a theoretical standpoint and therefore, provide a natural mechanism to test the propertie