SIMULATIONS OF MAGNETIC FIELDS IN CLUSTERS AND FILAMENTS
The origin of cosmic magnetic elds outside of galaxies remains controversial. In the intracluster medium eld strengths of the order of G have been reported. Possibly the out ows of AGN have magnetised the ICM. The intergalactic magnetic eld within laments should be less polluted by magnetised out ow...
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| Publié dans: | Revista Mexicana de Astronomía y Astrofísica |
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| Auteurs principaux: | , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Universidad Nacional Autónoma de México
2009
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| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57115743031 |
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