Origin of strong magnetic fields in Milky Way-like galaxies
2015 ◽
Vol 11
(S317)
◽
pp. 274-275
Keyword(s):
AbstractMagnetic 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).
2010 ◽
Vol 6
(S271)
◽
pp. 135-144
2008 ◽
Vol 4
(S259)
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pp. 529-538
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1980 ◽
Vol 296
(1419)
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pp. 339-345
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2016 ◽
Vol 33
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2009 ◽
Vol 5
(S262)
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pp. 240-243
Keyword(s):
1989 ◽
Vol 571
(1 Texas Symposi)
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pp. 239-246