The answer is blowing in the wind: simulating the interaction of jets with dynamic cluster atmospheres
Open Access
- 1 November 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society: Letters
- Vol. 373 (1) , L65-L69
- https://doi.org/10.1111/j.1745-3933.2006.00243.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 27 references indexed in Scilit:
- The relation between accretion rate and jet power in X-ray luminous elliptical galaxiesMonthly Notices of the Royal Astronomical Society, 2006
- AGN Feedback and Cooling Flows: Problems with Simple Hydrodynamic ModelsThe Astrophysical Journal, 2006
- Breaking the hierarchy of galaxy formationMonthly Notices of the Royal Astronomical Society, 2006
- Active Galactic Nuclei Heating and Dissipative Processes in Galaxy ClustersThe Astrophysical Journal, 2005
- Hot bubbles from active galactic nuclei as a heat source in cooling-flow clustersNature, 2002
- [ITAL]Chandra[/ITAL] ACIS-S Observations of Abell 4059: Signs of Dramatic Interaction between a Radio Galaxy and a Galaxy ClusterThe Astrophysical Journal, 2002
- The Centaurus A Northern Middle Lobe as a Buoyant BubbleThe Astrophysical Journal, 2001
- A Cosmic Double Helix in the Archetypical Quasar 3C273Science, 2001
- Shocks and Sonic Booms in the Intracluster Medium: X-Ray Shells and Radio Galaxy ActivityThe Astrophysical Journal, 2001
- Unusual Radio Structures in the Cooling Flow Cluster 2A 0335+096The Astrophysical Journal, 1995