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The large-scale structure of 3C 31

Abstract:
The results of a multifrequency VLA imaging study of the nearby radio galaxy 3C 31 are briefly summarized. The transition between jets and lobes is much more complex than was apparent from earlier observations, and is associated with significant variations in spectral index. We demonstrate that the known depolarization asymmetry in 3C 31 is caused by foreground Faraday rotation in the halo of the host galaxy, but the details of the associated field and density structure are not yet clear.
Publication status:
Published

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Journal:
PARTICLES AND FIELDS IN RADIO GALAXIES
Volume:
250
Pages:
437-442
Publication date:
2002-01-01
Event title:
Oxford Radio Galaxy Workshop
Source identifiers:
26401
ISBN:
1583810900
Keywords:
Pubs id:
pubs:26401
UUID:
uuid:8aec26c0-e87b-4fe8-b2c9-36b9ac07d3e9
Local pid:
pubs:26401
Deposit date:
2012-12-19

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