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Magnetised winds in dwarf galaxies

2009/08/31 by Y. Dubois, Yohan Dubois, Romain Teyssier +1 · 3 citations
Engineering · Physics and Astronomy · #Active galactic nucleus #Astronomy and Astrophysical Research #Cluster (spacecraft) #Dwarf galaxy #Electrical and Electromagnetic Research #Epoch (astronomy) #Field (mathematics) #Galaxy #Magnetic field #Magnitude (astronomy) #Space Technology and Applications #astro-ph.CO

paper · pdf · doi:10.1051/0004-6361/200913014

20 pages, 12 figures. Accepted for publication in A&A

arxiv created 2010/07/09 · openalex publication_date 2010/07/21 · arxiv updated 2015/05/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The generation and the amplification of magnetic fields in the current cosmological paradigm are still open questions. The standard theory is based on an early field generation by Biermann battery effects, possibly at the epoch of reionisation, followed by a long period of field amplification by galactic dynamos. The origin and the magnitude of the inter-galactic magnetic field is of primordial importance in this global picture, as it is considered to be the missing link between galactic magnetic fields and cluster magnetic fields on much larger scales.

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