Journal article
A young, dusty, compact radio source within a Lyα halo
- Abstract:
-
We report here on the discovery of a red quasar, J004929.4+351025.7 at a redshift of z = 2.48, situated within a large Lya emission-line halo. The radio spectral energy distribution implies that the radio jets were triggered < 10^4 years prior to the time at which the object is observed, suggesting that the jet triggering of the active galactic nucleus is recent. The loosely biconical structure of the emission-line halo suggests that it is ionised by photons emitted by the central quasar n...
Expand abstract
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(pdf, 2.8MB)
-
- Publisher copy:
- 10.1111/j.1365-2966.2008.13576.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
Funding
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 389
- Issue:
- 2
- Pages:
- 792-798
- Publication date:
- 2008-06-23
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Source identifiers:
-
16196
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:16196
- UUID:
-
uuid:048e1ca3-be2e-41f2-a43a-872b289e6679
- Local pid:
- pubs:16196
- Deposit date:
- 2012-12-19
Terms of use
- Copyright holder:
- Barrio et al
- Copyright date:
- 2008
- Notes:
- This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2008 Barrio et al. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
If you are the owner of this record, you can report an update to it here: Report update to this record