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Origin of strong magnetic fields in Milky Way-like galaxies

Published online by Cambridge University Press:  09 May 2016

Alexander M. Beck
Alexander M. Beck*
Affiliation:
University Observatory Munich Scheinerstr. 1, D-81679 Munich, Germany email: [email protected]
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Abstract

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Magnetic fields are observed on all scales in the Universe (see e.g. Kronberg 1994), but little is known about the origin and evolution of those fields with cosmic time. Seed fields of arbitrary source must be amplified to present-day values and distributed among cosmic structures. Therefore, the emergence of cosmic magnetic fields and corresponding dynamo processes (see e.g. Zel'dovich et al. 1983; Kulsrud et al. 1997) can only be jointly understood with the very basic processes of structure and galaxy formation (see e.g. Mo et al. 2010).

Keywords

methods: numericalgalaxies: formationgalaxies: magnetic fieldsearly Universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Issue S317: The General Assembly of Galaxy Halos: Structure, Origin and Evolution , August 2015 , pp. 274 - 275
Copyright
Copyright © International Astronomical Union 2016 

References

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