Conference icon

Conference

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

Actions


Authors


Feretti, L More by this author
Giovannini, G More by this author
Expand authors...
Volume:
250
Pages:
437-442
Publication date:
2002
URN:
uuid:8aec26c0-e87b-4fe8-b2c9-36b9ac07d3e9
Source identifiers:
26401
Local pid:
pubs:26401
ISBN:
1-58381-090-0
Keywords:

Terms of use


Metrics



If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP