Magnetic fields during high redshift structure formation

We explore the amplification of magnetic fields in the high-redshift Universe. For this purpose, we perform high-resolution cosmological simulations following the formation of primordial halos with ∼ ⊙ 107 M, revealing the presence of turbulent structures and complex morphologies at resolutions of a...

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Bibliographic Details

Main Authors:	Schleicher, Dominik R. G. (Author) , Latif, M. (Author) , Schober, Jennifer (Author) , Schmidt, W. (Author) , Bovino, S. (Author) , Federrath, C. (Author) , Niemeyer, J. (Author) , Banerjee, R. (Author) , Klessen, Ralf S. (Author)
Format:	Article (Journal)
Language:	English
Published:	2013 Jul 1
In:	Astronomische Nachrichten Year: 2013, Volume: 334, Issue: 6, Pages: 531-536
ISSN:	1521-3994
DOI:	10.1002/asna.201211898
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1002/asna.201211898 Verlag, lizenzpflichtig, Volltext: https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.201211898
Author Notes:	D.R.G. Schleicher, M. Latif, J. Schober, W. Schmidt, S. Bovino, C. Federrath, J. Niemeyer, R. Banerjee, and R.S. Klessen