2000/10/25 by Åke Nordlund, A . Nordlund, Nordlund, A . +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0010499
3 pages, 2 figures, to appear in `The origins of galactic magnetic fields', Proc. of JD14 of 23rd GA of the IAU, eds. D.Moss, R.Beck, A.Shukurov, in Highlights of Astronomy, vol. 12, ed. H.Rickman
arxiv created 2000/10/25 · openalex publication_date 2000/10/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We have studied the fate of initial magnetic fields in the hot halo gas out of which the visible parts of galaxies form, using three-dimensional numerical MHD-experiments. The halo gas undergoes compression by several orders of magnitude in the subsonic cooling flow that forms the cold disk. The magnetic field is carried along and is amplified considerably in the process, reaching muG levels for reasonable values of the initial ratio of magnetic to thermal energy density.