- Abstract:
-
We have analyzed the optical and radio properties of a sample of 3CR FR I radio galaxies which have Hubble Space Telescope imaging capable of detecting optical cores. The jet powers of the FR I radio galaxies are estimated from their low-frequency radio luminosities, and the optical core luminosity is taken as an upper limit on the emission from any unobscured accretion disc. We argue that if the accretion discs in these sources are assumed to be advection dominated accretion flows (ADAFs), o...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2004.07608.x
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- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 349
- Issue:
- 4
- Pages:
- 1419
- Publication date:
- 2003-12-16
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:62ecb8a8-887e-460d-9358-d262d429eeb0
- Source identifiers:
-
7331
- Local pid:
- pubs:7331
- Keywords:
- Copyright date:
- 2003
- Notes:
- A short note is added on 3C386 to match the published version
Journal article
No evidence for a different accretion mode for all 3CR FR I radio galaxies
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