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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