A three-phase amplification of the cosmic magnetic field in galaxies
Arguably the main challenge of galactic magnetism studies is to explain how the interstellar medium of galaxies reaches energetic equipartition despite the extremely weak cosmic primordial magnetic fields that are originally predicted to thread the inter-galactic medium. Previous numerical studies o...
| Päätekijät: | , , , |
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| Aineistotyyppi: | Journal article |
| Julkaistu: |
Oxford University Press
2018
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