- Abstract:
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I bring together evidence for the rapidity with which quasars' radio synchrotron lobe emission fades and for the intermittency with which jet plasma is ejected from individual quasars and radio galaxies and affirm the picture presented by Nipoti et al (2005) that the radio-loudness of quasars is a function of the epoch at which they are observed. I briefly illustrate this account with examples of successive episodes of jet activity where the axis along which jet plasma is launched appears to ...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Author's Original
- Files:
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(pdf, 437.7KB)
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- Publisher:
- Astronomical Society of the Pacific Publisher's website
- Journal:
- Extragalactic Jets: Theory and Observation from Radio to Gamma Ray Journal website
- Volume:
- 386
- Issue:
- 2
- Pages:
- 467–476
- Publication date:
- 2008-06-05
- Pubs id:
-
pubs:211837
- URN:
-
uri:921f4a7e-f35c-4a54-b9f8-767f7ee86261
- UUID:
-
uuid:921f4a7e-f35c-4a54-b9f8-767f7ee86261
- Local pid:
- pubs:211837
- Paper number:
- 2
- Keywords:
- Copyright holder:
- Astronomical Society of the Pacific
- Copyright date:
- 2008
- Notes:
-
This is a
pre-print version of a conference paper published by Astronomical Society of the Pacific in Extragalactic Jets: Theory and Observation from Radio to Gamma Ray in 2008-06, available online: http://adsabs.harvard.edu/abs/2008ASPC..386..467B
Journal article
Radio-loud and radio-quiet quasars: one population, different epochs of observation
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