X-Ray Variability of AGN and Relationship to Galactic Black Hole Binary Systems

Details X-Ray Variability of AGN and Relationship to Galactic Black Hole Binary Systems X-Ray Variability of AGN and Relationship to Galactic Black Hole Binary Systems

2009-09-14

arxiv.org/abs/0909.2579v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

28 pages, 13 figures, To appear in Belloni, T. (ed.): The Jet Paradigm - From Microquasars to Quasars, Lect. Notes Phys. 794 (

Scientific paper

Over the last 12 years, AGN monitoring by RXTE, has revolutionised our understanding of the X-ray variability of AGN, of the relationship between AGN and Galactic black hole X-ray binaries (BHBs) and hence of the accretion process itself, which fuels the emission in AGN and BHBs and is the major source of power in the universe. In this paper I review our current understanding of these topics. I begin by considering whether AGN and BHBs show the same X-ray spectral-timing `states' (e.g. low-flux, hard-spectrum or `hard' and high-flux, soft-spectrum or `soft'). Observational selection effects mean that most of the AGN which we have monitored will probably be `soft state' objects, but AGN are found in the other BHB states, although possibly with different critical transition accretion rates. I examine timescale scaling relationships between AGN and BHBs. I show that characteristic power spectral `bend' timescales, T_B, scale approximately with black hole mass, M_BH, but inversely with accretion rate, mdot_E, (in units of the Eddington accretion rate) probably signifying that T_B, arises at the inner edge of the accretion disc. The relationship T_B proportional to M_BH/mdot_E is a good fit, implying that no other potential variable, e.g. black hole spin, varies significantly. Lags between hard and soft X-ray bands as a function of Fourier timescale follow similar patterns in AGN and BHBs. [Abridged]

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