Radio Properties of Cavities in the ICM: Imprints of AGN Activity
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- 1 January 2007
- book chapter
- Published by Springer Nature
- p. 115-120
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This publication has 12 references indexed in Scilit:
- Breaking the hierarchy of galaxy formationMonthly Notices of the Royal Astronomical Society, 2006
- Radio bubbles in clusters of galaxiesMonthly Notices of the Royal Astronomical Society, 2005
- Particle energies and filling fractions of radio bubbles in cluster coresMonthly Notices of the Royal Astronomical Society, 2004
- A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and GalaxiesThe Astrophysical Journal, 2004
- What Shapes the Luminosity Function of Galaxies?The Astrophysical Journal, 2003
- The properties of the X-ray holes in the intracluster medium of the Perseus clusterMonthly Notices of the Royal Astronomical Society, 2002
- X-ray imaging-spectroscopy of Abell 1835Astronomy & Astrophysics, 2001
- Unification of the Radio and Optical Properties of Gigahertz Peak Spectrum and Compact Steep‐Spectrum Radio SourcesThe Astrophysical Journal, 1997
- Ageing and speeds in a representative sample of 21 classical double radio sourcesMonthly Notices of the Royal Astronomical Society, 1987
- Synchrotron aging in the lobes of luminous radio galaxiesThe Astrophysical Journal, 1985