AGN outflows and the cluster cooling flow conundrum
Temperature distributions within cores of galaxy clusters indicate gas in the core should cool down rapidly and contract. The cooling flow problem involves the hypothesis that the rapidly cooling gas should eventually condensate into unobserved molecular clouds. Active galactic nuclei (AGNs) are tho...
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University of Southampton
2011
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.538974 |