- 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
- Version:
- Publisher's version
- Files:
-
-
(pdf, 2.8mb)
-
- Publisher copy:
- 10.1111/j.1365-2966.2008.13576.x
-
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- 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
- URN:
-
uuid:048e1ca3-be2e-41f2-a43a-872b289e6679
- Source identifiers:
-
16196
- Local pid:
- pubs:16196
- Language:
- English
- Keywords:
- 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.
Journal article
A young, dusty, compact radio source within a Lyα halo
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