SIMBAD references

2007MNRAS.381..741P - Mon. Not. R. Astron. Soc., 381, 741-746 (2007/October-3)

Rapidly varying accretion and AGN feedback.

POPE E.C.D.

Abstract (from CDS):

Accretion rates on to active galactic nuclei (AGNs) are likely to be extremely variable on short time-scales; much shorter than the typical cooling time of X-ray emitting gas in elliptical galaxies and galaxy clusters. Using the Langevin approach it is shown that, for a simple feedback system, this can induce variability in the AGN power output that is of much larger amplitude, and persists for longer time-scales, than the initial fluctuations. An implication of this is that rich galaxy clusters are expected to show the largest and longest-lived fluctuations. Stochastic variations in the accretion rate also mean that the AGN injects energy across a wide range of time-scales. This allows the AGN to maintain a much closer balance with its surroundings than if it was periodically activated. The possible non-linear correlation between Bondi accretion rate and jet power, found by Allen et al., can be explained if the instantaneous accretion rate, scaled by jet power, varies log-normally. This explanation also implies that the duty cycle of AGN activity increases with the radiative losses of the surroundings, in qualitative agreement with Best et al.

Abstract Copyright: 2007 The Author. Journal compilation © 2007 RAS

Journal keyword(s): galaxies: active - galaxies: cooling flows - galaxies: jets

Status at CDS:  

Simbad objects: 1

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2020.04.09-10:01:23

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