A massive, cooling-flow-induced starburst in the core of a highly luminous cluster of galaxies
In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the cluster’s lifetime, leading to continuous ‘cooling flows’ of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formatio...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Nature Publishing Group
2014
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| Online Access: | http://hdl.handle.net/1721.1/88548 https://orcid.org/0000-0002-1379-4482 https://orcid.org/0000-0003-3769-9559 |