
Extragalactic
radio sources
(continued)
- The lobes:
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Fig 1:
Radio emission (in orange) superposed to optical emission (in blue) of NGC 1316 .
Although the symmetrical structure is preserved,
neither the radio nucleus nor the jet are visible. The hypothesis is
that the central motor of the radio source (black hole ) has exhausted
its fuel.
(Credits: NRAO)
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The Webweavers: Last modified Mon, 22 Mar 2004 10:04:07 GMT
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