Journal article
No evidence for a different accretion mode for all 3CR FR I radio galaxies
- 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
Actions
Access Document
- Publisher copy:
- 10.1111/j.1365-2966.2004.07608.x
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- 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
Item Description
- Keywords:
Terms of use
- Copyright date:
- 2003
- Notes:
- A short note is added on 3C386 to match the published version
If you are the owner of this record, you can report an update to it here: Report update to this record