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Extragalactic magnetic fields

Kronberg, P P·1994·Reports on Progress in Physics
DOI 10.1088/0034-4885/57/4/001
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Abstract

The observational methods for detecting and measuring extragalactic magnetic fields are discussed, along with some new indirect methods which could be used for inferring field strengths at large redshifts which are otherwise beyond the reach of direct measurement. Various cosmological seed field generation mechanisms are reviewed, which could generate seed fields for the subsequently formed galaxies. The question of whether the original seed fields were produced in galaxies, or the pre-recombination early Universe must await a clearer picture of how the first stars and galaxies formed.

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Metadata

Authors
Kronberg, P. P.
Venue
Reports on Progress in Physics
Publisher
IOP Publishing
Published
1994-04-01
Volume
57
Issue
4
Pages
325-382
ISSN
  • 0034-4885 (ISSN-L)
  • 1361-6633
DOI
10.1088/0034-4885/57/4/001
OpenAlex
W2016951470
Cited by
1,015
References
3
FWCI
30.97
Type
journal article
Language
en
Open access
closed

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