A diffuse bubble-like radio-halo source MRC 0116+111: imprint of AGN feedback in a low-mass cluster of galaxies
- 21 October 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 399 (2) , 601-614
- https://doi.org/10.1111/j.1365-2966.2009.15310.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 71 references indexed in Scilit:
- Radiative Efficiency and Content of Extragalactic Radio Sources: Toward a Universal Scaling Relation between Jet Power and Radio PowerThe Astrophysical Journal, 2008
- Giant Ringlike Radio Structures Around Galaxy Cluster Abell 3376Science, 2006
- The relation between accretion rate and jet power in X-ray luminous elliptical galaxiesMonthly Notices of the Royal Astronomical Society, 2006
- A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and GalaxiesThe Astrophysical Journal, 2004
- Proton-synchrotron radiation of large-scale jets in active galactic nucleiMonthly Notices of the Royal Astronomical Society, 2002
- The new emerging model for the structure of cooling cores in clusters of galaxiesAstronomy & Astrophysics, 2002
- [ITAL]Chandra[/ITAL] Observation of the Radio Source/X-Ray Gas Interaction in the Cooling Flow Cluster Abell 2052The Astrophysical Journal, 2001
- Evolving cooling flowsMonthly Notices of the Royal Astronomical Society, 1995
- A new catalog of 53,522 4.85 GHz sourcesThe Astrophysical Journal Supplement Series, 1991
- Theory of extragalactic radio sourcesReviews of Modern Physics, 1984