| dc.contributor.author | Shabala, S. | |
| dc.contributor.author | Kaviraj, S. | |
| dc.contributor.author | Silk, J. | |
| dc.date.accessioned | 2014-10-02T11:30:51Z | |
| dc.date.available | 2014-10-02T11:30:51Z | |
| dc.date.issued | 2012-08 | |
| dc.identifier.citation | Shabala , S , Kaviraj , S & Silk , J 2012 , ' Effects of large-scale AGN feedback in local galaxies ' , Proceedings of the International Astronomical Union , vol. 8 , no. S292 , pp. 375 . https://doi.org/10.1017/S1743921313001762 | |
| dc.identifier.issn | 1743-9213 | |
| dc.identifier.other | ORCID: /0000-0002-5601-575X/work/77850187 | |
| dc.identifier.uri | http://hdl.handle.net/2299/14528 | |
| dc.description.abstract | The effects of active galactic nucleus (AGN) feedback on group and cluster galaxies are investigated. We examine the colors of non-AGN hosts (i.e. satellite galaxies) by comparing galaxies overrun by radio AGN with similar galaxies located outside the radio AGN contours. We find that powerful Fanaroff-Riley type II (edge-brightened) radio AGN truncate star formation in the galaxies overrun by AGN-driven bow shocks. On the other hand, the ubiquitous Fanaroff-Riley type I (core-dominated) AGN do not affect neighboring galaxies. This result shows that, despite their rarity, feedback from powerful radio AGN is an important factor in the evolution of group/cluster galaxies. | en |
| dc.format.extent | 1 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Proceedings of the International Astronomical Union | |
| dc.title | Effects of large-scale AGN feedback in local galaxies | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.description.status | Non peer reviewed | |
| rioxxterms.versionofrecord | 10.1017/S1743921313001762 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
