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Cooling flows or warming rays?
The radiative cooling time of the X-ray-emitting plasma near the center in many clusters of galaxies is shorter than the age of the cluster, but neither the expected large drop in central temperature --nor the expected mass flow towards the pressure-depleted cluster centers-- are observed. We propos...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2003
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1051/0004-6361:20031509 http://cds.cern.ch/record/614108 |