Bubbles as tracers of heat input to cooling flows
Open Access
- 2 April 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 377 (1) , 142-146
- https://doi.org/10.1111/j.1365-2966.2007.11575.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 26 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-controlled cooling in elliptical galaxiesMonthly Notices of the Royal Astronomical Society: Letters, 2006
- Black holes, cuspy atmospheres and galaxy formationPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2005
- A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and GalaxiesThe Astrophysical Journal, 2004
- XMM‐NewtonObservations of the Perseus Cluster. I. The Temperature and Surface Brightness StructureThe Astrophysical Journal, 2003
- The long-term effect of radio sources on the intracluster mediumMonthly Notices of the Royal Astronomical Society, 2003
- Cooling flows as a calorimeter of active galactic nucleus mechanical powerMonthly Notices of the Royal Astronomical Society, 2002
- Simulation of radio plasma in clusters of galaxiesMonthly Notices of the Royal Astronomical Society, 2002
- A High‐Resolution Study of the Hydra A Cluster withChandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling FlowThe Astrophysical Journal, 2001
- A ROSAT HRI study of the interaction of the X-ray-emitting gas and radio lobes of NGC 1275Monthly Notices of the Royal Astronomical Society, 1993