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2006MNRAS.372.1840R - Mon. Not. R. Astron. Soc., 372, 1840-1850 (2006/November-2)
Effect of turbulent diffusion on iron abundance profiles.
REBUSCO P., CHURAZOV E., BOHRINGER H. and FORMAN W.
Abstract (from CDS):
We also estimated the characteristic velocities and the spatial scales of the gas motions needed to balance the cooling losses by the dissipation of the same gas motions. A comparison of the derived spatial scales and the sizes of observed radio bubbles inflated in the ICM by a central active galactic nucleus (AGN) suggests that the AGN/ICM interaction makes an important (if not a dominant) contribution to the gas motions in the cluster cores.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): diffusion - turbulence - galaxies: abundances
Simbad objects: 15
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