How AGN feedback and metal cooling shape cluster entropy profiles
Observed clusters of galaxies essentially come in two flavors: non cool core clusters characterized by an isothermal temperature profile and a central entropy floor, and cool-core clusters where temperature and entropy in the central region are increasing with radius. Using cosmological resimulatio...
| Päätekijät: | , , , |
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| Aineistotyyppi: | Journal article |
| Julkaistu: |
Oxford University Press
2011
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