Diffuse Radio Emission from Galaxy Clusters
arXiv:1901.04496 · doi:10.1007/s11214-019-0584-z
Abstract
In a growing number of galaxy clusters diffuse extended radio sources have been found. These sources are not directly associated with individual cluster galaxies. The radio emission reveal the presence of cosmic rays and magnetic fields in the intracluster medium (ICM). We classify diffuse cluster radio sources into radio halos, cluster radio shocks (relics), and revived AGN fossil plasma sources. Radio halo sources can be further divided into giant halos, mini-halos, and possible `intermediate' sources. Halos are generally positioned at cluster center and their brightness approximately follows the distribution of the thermal ICM. Cluster radio shocks (relics) are polarized sources mostly found in the cluster's periphery. They trace merger induced shock waves. Revived fossil plasma sources are characterized by their radio steep-spectra and often irregular morphologies. In this review we give an overview of the properties of diffuse cluster radio sources, with an emphasis on recent observational results. We discuss the resulting implications for the underlying physical acceleration processes that operate in the ICM, the role of relativistic fossil plasma, and the properties of ICM shocks and magnetic fields. We also compile an updated list of diffuse cluster radio sources which will be available on-line http://galaxyclusters.com. We end this review with a discussion on the detection of diffuse radio emission from the cosmic web.
To appear in Space Science Reviews, 56 pages, 31 figures; For associated data see http://galaxyclusters.com
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- How unusual is the cool-core radio halo cluster CL1821+643 ?
- The origin of the diffuse non-thermal X-ray and radio emission in the Ophiuchus cluster of galaxies
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- PITSZI: Probing Intra-cluster medium Turbulence with Sunyaev-Zel'dovich Imaging -- Application to the triple merging cluster MACS J0717.5+3745
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- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
- Jet interaction with galaxy cluster mergers
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- Sloshing and spiral structures breeding a putative radio mini-halo in the environment of a cool-core cluster Abell 795
- Abell 0399-Abell 0401 radio bridge spectral index: the first multifrequency detection
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- Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
- Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
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- A spectroscopic survey of Abell 1703: is it a rare relaxed cluster hosting a radio halo or a usual merging system?
- Cluster outskirts and their connection to the cosmic web
- Magnetic fields and extraordinarily bright radio emission in the X-ray faint galaxy group MRC 0116+111
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- CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
- Galactic Traversability: A New Concept for Extragalactic SETI
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- Possible non-thermal origin of the hard X-ray emission in the merging galaxy cluster SPT-CL J2031-4037
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- Deep Chandra observations of PLCKG287.0+32.9: a clear detection of a shock front in a heated former cool core
- Cosmic-ray electrons and the magnetic field of the North Polar Spur
- Energy Dissipation in Strong Collisionless Shocks: The Crucial Role of Ion-to-Electron Scale Separation in Particle-in-Cell Simulations
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- Post-processing of galaxies due to major cluster mergers I. hints from galaxy colours and morphologies
- Optical/X-ray/radio view of Abell 1213: A galaxy cluster with anomalous diffuse radio emission
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- Revisiting the Dragonfly Galaxy I. High-resolution ALMA and VLA Observations of the Radio Hotspots in a Hyper-luminous Infrared Galaxy at
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- Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
- Fast and "lossless" propagation of relativistic electrons along magnetized non-thermal filaments in galaxy clusters and the Galactic Center region
- The Coma cluster at LOFAR frequencies II: the halo, relic, and a new accretion relic
- Simulated Rotation Measure Sky from Primordial Magnetic Fields
- VLBI Detection of an Active Radio Source Potentially Driving 100-kpc Scale Emission in the Ultraluminous Infrared Galaxy IRAS F010042237
- The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
- Somewhere in between: Tracing the Radio Emission from Galaxy Groups (or Why Does the Future of Observing Galaxy Groups with Radio Telescopes Look Promising?)
- Plasma Constraints on the Millicharged Dark Matter
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- The Complexity and Information Content of Simulated Universes
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- Galaxy-cluster-stacked Fermi-LAT II: extended central hadronic signal
- The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11
- Discovery of large-scale radio emission enveloping the mini-halo in the most X-ray luminous galaxy cluster RX~J1347.5-1145
- Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351
- Radio halos in a mass-selected sample of 75 galaxy clusters. I. Sample selection and data analysis
- Witnessing a Galaxy Cluster Merger with JWST and a Chandra X-ray Temperature Map
- Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
- Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
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- Enhanced radio emission between a galaxy cluster pair
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- Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data
- Cool-core, X-ray cavities and cold front revealed in RXCJ0352.9+1941 cluster by Chandra and GMRT observations
- Small-scale dynamo with finite correlation times
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- Acceleration of cosmic rays by double shock waves in galaxy clusters: application to radio relics
- MOSS I: Double radio relics in the Saraswati supercluster
- Relativistic ions with power-law spectra explain radio phoenixes
- On the Origin of Diffuse Radio Emission in Abell 85 -- Insights from new GMRT Observations
- Particle Reacceleration by Turbulence and Radio Constraints on Multi-Messenger High-Energy Emission from the Coma Cluster
- The mechanism of efficient electron acceleration at parallel non-relativistic shocks
- Power-law Spectrum of Energetic Particles in Classical Thermal Equilibrium by Pitch-angle Scattering Process
- The structure of cluster merger shocks: turbulent width and the electron heating timescale
- Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP
- A Model of EUV Emission from Clusters of Galaxies
- Constraints on dark matter annihilation and turbulent reacceleration set by high-frequency observations of the radio halo in the Coma cluster
- A LOFAR-uGMRT spectral index study of distant radio halos
- MIGHTEE: total intensity radio continuum imaging and the COSMOS / XMM-LSS Early Science fields
- Probing the evolution of galaxy clusters using SZ effect and non-thermal emission: first results from A1413
- Observations of the galaxy cluster CL 0217+70 and its surrounding region at 1.4 GHz with the Sardinia Radio Telescope
- Radially polarized synchrotron from galaxy-cluster virial shocks
- Probing AGN duty cycle and cluster-driven morphology in a giant episodic radio galaxy
- A new shock in the pre-merging cluster pair 1E2215-2216
- Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications
- Evidence of sloshing-driven mini-halo formation in the cool-core cluster RXCJ1558.3-1410
- The Optical Properties of Host Galaxies of Radio Sources in the Coma Cluster
- Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
- A high-resolution study of the double radio relic system in MACS J1752.0+4440
- The MeerKAT Massive Distant Clusters Survey: a search for diffuse radio emission in 30 massive SZ-selected clusters at
- Galaxy clusters in the LoTSS-DR3: Catalogues and detection pipeline for diffuse radio emission
- Multi-wavelength insights into the pulsar wind nebula candidate near 1LHAASO J0343+5254u: an obscured merging galaxy cluster?