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...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Ngā kaituhi matua: | , , , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2009
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57115743031 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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