Journal article
Active galactic nucleus feedback drives the colour evolution of local galaxies
- Abstract:
- We investigate the effects of active galactic nucleus (AGN) feedback on the colour evolution of galaxies found in local (z < 0.2) groups and clusters. Galaxies located within the lobes of powerful Fanaroff-Riley type II (FR II) (edge-brightened) sources show much redder colours than neighbouring galaxies that are not spatially coincident with the radio source. By contrast, no similar effect is seen near FR I (core-dominated) radio sources. We show that these colours are consistent with FR II sources truncating star formation as the expanding bow shock overruns a galaxy. We examine a sample of clusters with no detectable radio emission and show that galaxy colours in these clusters carry an imprint of past AGN feedback. The AGN activity in the low-redshift Universe is predominantly driven by low-luminosity radio sources with short duty cycles. Our results show that, despite their rarity, feedback from powerful radio sources is an important driver of galaxy evolution even in the local volume.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
- Publisher:
- Wiley-Blackwell
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 413
- Issue:
- 4
- Pages:
- 2815-2826
- Publication date:
- 2011-01-01
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Language:
-
English
- Keywords:
- Subjects:
- UUID:
-
uuid:ab05fe14-06aa-4ae1-ac2a-b8d92f45a8d0
- Local pid:
-
ora:5386
- Deposit date:
-
2011-05-27
Terms of use
- Copyright holder:
- S S Shabala, S Kaviraj & J Silk
- Copyright date:
- 2011
- Notes:
- Citation: Shabala, S. S., Kaviraj, S. & Silk, J. (2011). 'Active galactic nucleus feedback drives the colour evolution of local galaxies', Monthly Notices of the Royal Astronomical Society 413(4), 2815-2826. [The definitive version of the article is available at http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2011.18353.x/abstract]. © 2011 Authors. The full-text of this article is not available in ORA, but you may be able to access the article via the publisher copy link on this record page.
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