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 observe...
Main Authors: | McDonald, Michael A. (Contributor), Bautz, Marshall W. (Contributor), Simcoe, Robert A. (Contributor), Sullivan, Peter W. (Author), Miller, Eric D (Author) |
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Other Authors: | Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), Sullivan, P. (Contributor), Miller, Eric D. (Contributor) |
Format: | Article |
Language: | English |
Published: |
Nature Publishing Group,
2014-08-06T17:33:23Z.
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Subjects: | |
Online Access: | Get fulltext |
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