- Abstract:
-
The hot (10(7) to 10(8) kelvin), X-ray-emitting intracluster medium (ICM) is the dominant baryonic constituent of clusters of galaxies. In the cores of many clusters, radiative energy losses from the ICM occur on timescales much shorter than the age of the system. Unchecked, this cooling would lead to massive accumulations of cold gas and vigorous star formation, in contradiction to observations. Various sources of energy capable of compensating for these cooling losses have been proposed, th...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1038/nature13830
-
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- Journal:
- Nature
- Volume:
- 515
- Issue:
- 7525
- Pages:
- 85-87
- Publication date:
- 2014-11-05
- DOI:
- EISSN:
-
1476-4687
- ISSN:
-
0028-0836
- URN:
-
uuid:e375866a-52f0-4598-ba3d-4f571ad1cc4f
- Source identifiers:
-
489849
- Local pid:
- pubs:489849
- Language:
- English
- Keywords:
- Copyright date:
- 2014
- Notes:
- published in Nature
Journal article
Turbulent heating in galaxy clusters brightest in X-rays.
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