期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 342, 期 2, 页码 463-466出版社
OXFORD UNIV PRESS
DOI: 10.1046/j.1365-8711.2003.06548.x
关键词
galaxies : clusters : general; cooling flows; intergalactic medium; X-rays : galaxies : clusters
I use a simple analytical model to show that simple heat conduction models cannot significantly suppress cluster cooling flows. I build a static medium where heat conduction globally balances radiative cooling, and then perturb it. I show that a perturbation extending over a large fraction of the cooling flow region and with an amplitude of similar to10 per cent, will grow to the non-linear regime within a Hubble time. Such perturbations are reasonable in clusters that frequently experience mergers and/or active galactic nuclei activity. This result strengthens previous findings which show that a steady solution does not exist for a constant heat conduction coefficient.
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