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9 - Magnetic fields associated with clusters and groups of galaxies

Published online by Cambridge University Press:  22 September 2016

Philipp P. Kronberg
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University of Toronto
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References

Abell, G. O. 1958, The Distribution of Rich Clusters of Galaxies, Astrophys. J. Suppl., 3, 211CrossRefGoogle Scholar
Abramopoulos, F. & Ku, W. H.-M. 1983, X-Ray Survey of Clusters of Galaxies with the Einstein Observatory, Astrophys. J., 271, 446CrossRefGoogle Scholar
Aharonian, F. A., Akhperjanian, A. D., Anton, G., et al. (The H.E.S.S. Collaboration). 2009, Constraints on the Multi-TeV Particle Population in the Coma Galaxy Cluster with HESS Observations, Astron. Astrophys., 502, 437CrossRefGoogle Scholar
Binney, J. J. 1998, M 87 and Cooling Flows, in The Radio Galaxy Messier 87: Proceedings of a Workshop Held at Ringberg Castle, Tegernsee, Germany, 15–19 September 1997, eds. Röser, H. J. & Meisenheimer, K., Lecture Notes in Physics (Berlin: Springer), 530, 116Google Scholar
Birkinshaw, M. 1999, The Sunyaev-Zel’dovich Effect, Phys. Rep., 310, 97CrossRefGoogle Scholar
Blumenthal, G. R., & Gould, R. J. 1970, Bremsstrahlung, Synchrotron Radiation, and Compton Scattering of High-Energy Electrons Traversing Dilute Gases, Rev. Mod. Phys., 42, 237CrossRefGoogle Scholar
Brentjens, M. & deBruyn, G. 2006, RM-Synthesis of the Perseus Cluster, Astron. Nachrichten, 327, 545CrossRefGoogle Scholar
Briel, U. G., Henry, J. P., & Böhringer, H. 1992, Observation of the Coma Cluster of Galaxies with ROSAT During the All-Sky Survey, Astron. Astrophys., 259, L31Google Scholar
Brunetti, G., Blasi, P., Cassano, R., & Gabici, S. 2004, Alfvénic Reacceleration of Relativistic Particles in Galaxy Clusters: MHD Waves, Leptons and Hadrons, MNRAS, 350, 1174Google Scholar
Burbidge, G. R. 1956, On Synchrotron Radiation from Messier 87, Astrophys. J., 124, 416CrossRefGoogle Scholar
Burn, B. J. 1966, On the Depolarization of Discrete Radio Sources by Faraday Dispersion, MNRAS, 133, 67CrossRefGoogle Scholar
Butcher, H. & Oemler, A. 1978, The Evolution of Galaxies in Clusters. II – The Galaxy Content of Nearby Clusters, Astrophys. J., 226, 559CrossRefGoogle Scholar
Carlberg, R. G., Yee, H. Y. C., & Ellingson, E. 1997, The Average Mass and Light Profiles of Galaxy Clusters, Astrophys. J., 478, 462CrossRefGoogle Scholar
Cho, J. & Ryu, D. 2009, Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence, Astrophys. J., 705, L90CrossRefGoogle Scholar
Churazov, E., Forman, W., Jones, C., Sunyaev, R., & Böhringer, H. 2004, XMM-Newton Observations of the Perseus Cluster – II. Evidence for Gas Motions in the Core, MNRAS, 347, 29Google Scholar
Churazov, E., Sunyaev, R., Forman, W., & Böhringer, H. 2002, Cooling Flows as a Calorimeter of Active Galactic Nucleus Mechanical Power, MNRAS, 332, 729CrossRefGoogle Scholar
Chyžy, K. T., Soida, M., Bomans, D. J., Vollmer, B., Balkowski, Ch., Beck, R., & Urbanik, M. 2006, Large-Scale Magnetized Outflows from the Virgo Cluster Spiral NGC 4569: A Galactic Wind in a Ram Pressure Wind, Astron. Astrophys., 447, 465CrossRefGoogle Scholar
Clarke, D. A. 1993, 3-D MHD Simulations of Extragalactic Jets, in Jets in Extragalactic Radio Sources: Proceedings of a Workshop Held at Ringberg Castle, Tegernsee, FRG September 22–28, 1991, ed. Röser, H.-J. & Meisenheimer, K., Lecture Notes in Physics (Berlin: Springer), 421, 243Google Scholar
Clarke, T. E., Kronberg, P. P., & Böhringer, H. 2001, A New Radio-X-Ray Probe of Galaxy Cluster Magnetic Fields, Astrophys. J., 547, L111CrossRefGoogle Scholar
Daly, R. A. & Loeb, A. 1990, A Possible Origin of Galactic Magnetic Fields, Astrophys. J., 364, 451CrossRefGoogle Scholar
De Young, D. S. 1992, Galaxy-Driven Turbulence and the Growth of Intracluster Magnetic Fields, Astrophys. J., 386, 464CrossRefGoogle Scholar
Dennison, B. 1980, Formation of Radio Halos in Clusters of Galaxies from Cosmic-Ray Protons, Astrophys. J., 239, L93CrossRefGoogle Scholar
Dermer, C. D. 1986, Binary Collision Rates of Relativistic Thermal Plasmas. II. Spectra, Astrophys. J., 307, 47CrossRefGoogle Scholar
Diehl, S., Li, H., Fryer, C. L., & Rafferty, D. 2008, Constraining the Nature of X-Ray Cavities in Clusters and Galaxies, Astrophys. J., 687, 173CrossRefGoogle Scholar
Dolag, K., Bartelmann, M., & Lesch, H. 1999, SPH Simulations of Magnetic Fields in Galaxy Clusters, Astron. Astrophys., 348, 351Google Scholar
Dreher, J. W., Carilli, C. L., & Perley, R. A. 1987, The Faraday Rotation of Cygnus A – Magnetic Fields in Cluster Gas, Astrophys. J., 316, 611CrossRefGoogle Scholar
Eilek, J. A. 1993, Dynamo-Supported Magnetic Fields in Radio Jets, in Jets in Extragalactic Radio Sources, Proceedings of a Workshop Held at Ringberg Castle, Tegernsee, FRG, September 22–28, 1991, ed. Röser, H.-J. & Meisenheimer, K., Lecture Notes in Physics (Berlin: Springer), 421, 131CrossRefGoogle Scholar
Enßlin, T. A. & Kaiser, C. R. 2000, Comptonization of the Cosmic Microwave Background by Relativistic Plasma, Astron. Astrophys., 360, 417Google Scholar
Enßlin, T. A. & Vogt, C. 2006, Magnetic Turbulence in Cool Cores of Galaxy Clusters, Astron. Astrophys., 453 , 447CrossRefGoogle Scholar
Fabian, A. C. 1999, Cooling Flows pre Chandra, XMM and ASTRO-E, in Diffuse Thermal and Relativistic Plasma in Galaxy Clusters, ed. Böhringer, H., Feretti, L., & Schuecker, P., MPE Report (Garching: Max-Planck-Institut für Extraterrestrische Physik) 271, 123Google Scholar
Felten, J. E. 1996, Mitigating the Baryon Crisis in Clusters: Can Magnetic Pressure be Important?, in Clusters, Lensing and the Future of the Universe, ed. Trimble, V. & Reisenegger, A., ASP Conf. Ser. (San Francisco: Astronomical Society of the Pacific), 88, 271Google Scholar
Felten, J. E. & Morrison, P. 1966, Omnidirectional Inverse Compton and Synchrotron Radiation from Cosmic Distributions of Fast Electrons and Thermal Photons, Astrophys. J., 146, 686CrossRefGoogle Scholar
Feretti, L., Dallacasa, D., Giovannini, G., & Tagliani, A. 1995, The Magnetic Field in the Coma Cluster, Astron. Astrophys., 302, 680Google Scholar
Feretti, L., Dallacasa, D., Govoni, F., Giovannini, G., Taylor, G. B., & Klein, U. 1999, The Radio Galaxies and the Magnetic Field in Abell 119, Astron. Astrophys., 344, 472Google Scholar
Garrington, S. T. & Conway, R. G. 1991, The Interpretation of Asymmetric Depolarization in Extragalactic Radio Sources, MNRAS, 250, 198CrossRefGoogle Scholar
Garrington, S. T., Leahy, J. P., Conway, R. G., & Laing, R. A. 1988, A Systematic Asymmetry in the Polarization Properties of Double Radio Sources with One Jet, Nature, 331, 147CrossRefGoogle Scholar
Goldman, I. & Rephaeli, Y. 1991, Turbulently Generated Magnetic Fields in Clusters of Galaxies, Astrophys. J., 380, 344CrossRefGoogle Scholar
Heald, G., Braun, R., & Edmonds, R. 2009, The Westerbork SINGS Survey. II Polarization, Faraday Rotation, and Magnetic Fields, Astron. Astrophys., 503, 409CrossRefGoogle Scholar
Heckman, T. M., Baum, S. A., van Breugel, W. J. M., & McCarthy, P. 1989, Dynamical, Physical, and Chemical Properties of Emission-Line Nebulae in Cooling Flows, Astrophys. J., 338, 48CrossRefGoogle Scholar
Henriksen, M. J. & Mushotzky, R. F. 1986, The X-Ray Spectrum of the Coma Cluster of Galaxies, Astrophys. J., 302, 287CrossRefGoogle Scholar
Hu, J. & Lou, Y.-Q. 2004, Magnetic Sunyaev-Zel’dovich Effect in Galaxy Clusters, Astrophys. J., 606, L1CrossRefGoogle Scholar
Jaffe, W. J. 1980, On the Morphology of the Magnetic Field in Galaxy Clusters, Astrophys. J., 241, 925CrossRefGoogle Scholar
Jaffe, W. J. & Perola, G. C. 1973, Dynamical Models of Tailed Radio Sources in Clusters of Galaxies, Astron. Astrophys., 26, 423Google Scholar
Kaiser, N. 2001, Weak Lensing by Galaxy Clusters, in Gravitational Lensing: Recent Progress and Future Goals, ed. Brainerd, T. G. & Kochanek, C. S., ASP Conf. Ser. (San Francisco: Astronomical Society of the Pacific), 237, 269Google Scholar
Kim, K.-T., Kronberg, P. P., Dewdney, P. E., & Landecker, T. L. 1990, The Halo and Magnetic Field of the Coma Cluster of Galaxies, Astrophys. J., 355, 29CrossRefGoogle Scholar
Kim, K.-T., Tribble, P. C., & Kronberg, P. P. 1991, Detection of Excess Rotation Measure Due to Intracluster Magnetic Fields in Clusters of Galaxies, Astrophys. J., 379, 80CrossRefGoogle Scholar
King, I. R. 1972, Density Data and Emission Measure for a Model of the Coma Cluster, Astrophys. J., 174, L123CrossRefGoogle Scholar
Kompaneets, A. S. 1956, The Establishment of Thermal Equilibrium Between Quanta and Electrons, Zh. Exper. Teor. Fiziki, 31, 876Google Scholar
Kulsrud, R. M., Cen, R., Ostriker, J. P., Ryu, D. 1997, The Protogalactic Origin for Cosmic Magnetic Fields, Astrophys. J., 480, 481CrossRefGoogle Scholar
Lane, W. M., Clarke, T. E., Taylor, G. B., Perley, R. A., & Kassim, N. E. 2004, Hydra A at Low Radio Frequencies, Astron. J., 127, 48CrossRefGoogle Scholar
Lawler, J. M. & Dennison, B. 1982, On Intracluster Faraday Rotation. II – Statistical Analysis, Astrophys. J.,252, 81CrossRefGoogle Scholar
Ohno, H., Takizawa, M., & Shibata, S. 2002, Radio Halo Formation through Magnetoturbulent Particle Acceleration in Clusters of Galaxies, Astrophys. J., 577, 658CrossRefGoogle Scholar
Owen, F., Eilek, J., & Kassim, N. 1999, M87: Outflow Not Cooling Flow?, in Diffuse Thermal and Relativistic Plasma in Galaxy Clusters: Proceedings of the Workshop...Ringberg Castle, Germany, April 19–23, 1999, ed. Bohringer, H., Feretti, L., & Schuecker, P., MPE Report (Garching, Germany: Max-Planck-Institut für Extraterrestrische Physik), 271, 107Google Scholar
Owen, F. N., Eilek, J. A., & Kassim, N. 2000, M87 at 90 Centimeters: A Different Picture, Astrophys. J., 543, 611CrossRefGoogle Scholar
Pacholczyk, A. G. 1970, Radio Astrophysics (San Francisco: W. H. Freeman & Co.)Google Scholar
Peres, C. B., Fabian, A. C., Edge, A. C., Allen, S. W., Johnstone, R. M., & White, D. A. 1998, A ROSAT Study of the Cores of Clusters of Galaxies – I. Cooling Flows in an X-Ray Flux-Limited Sample, MNRAS, 298, 416Google Scholar
Perley, R. A. & Taylor, G. B. 1991, VLA Observations of 3C 295 – A Young Radio Galaxy?, Astron. J., 101, 1623CrossRefGoogle Scholar
Pfrommer, C. & Enßlin, T. A. 2004a, Estimating Galaxy Cluster Magnetic Fields by the Classical and Hadronic Minimum Energy Criterion, MNRAS, 352, 76CrossRefGoogle Scholar
Pfrommer, C. & Enßlin, T. A. 2004b, Constraining the Population of Cosmic Ray Protons in Cooling Flow Clusters with γ-Ray and Radio Observations: Are Radio Mini-Halos of Hadronic Origin?, Astron. Astrophys., 413, 17CrossRefGoogle Scholar
Pfrommer, C. & Enßlin, T. A. 2004c, Erratum: Constraining the Population of Cosmic Ray Protons in Cooling Flow Clusters with γ-Ray And Radio Observations: Are Radio Mini-Halos of Hadronic Origin?, Astron. Astrophys., 426, 777CrossRefGoogle Scholar
Rephaeli, Y. 1995, Comptonization of the Cosmic Microwave Background: The Sunyaev-Zeldovich Effect, Ann. Rev. Astr. Astrophys., 33, 541CrossRefGoogle Scholar
Rephaeli, Y. & Gruber, D. E. 1988, HEAO 1 Hard X-Ray Observation of Clusters of Galaxies and Intracluster Magnetic Fields, Astrophys. J., 333, 133CrossRefGoogle Scholar
Reuter, H.-P., Klein, U., Lesch, H., Wielebinski, R., & Kronberg, P. P. 1994, The Magnetic Field in the Halo of M 82. Polarized Radio Emission at Lambda-Lambda(6.2) and 3.6 CM, Astron. Astrophys., 282, 724Google Scholar
Roettiger, K., Burns, J. O., & Stone, J. M. 1999, A Cluster Merger and the Origin of the Extended Radio Emission in Abell 3667, Astrophys. J., 518, 603CrossRefGoogle Scholar
Röttgering, H. J. B., Wieringa, M. H., Hunstead, R. W., & Ekers, R. D. 1997, The Extended Radio Emission in the Luminous X-Ray Cluster A3667, MNRAS, 290, 577CrossRefGoogle Scholar
Rood, H. 1970, Conversion from Measured Line-Of to Space-Velocity Dispersion for a Spherical Cluster of Galaxies: Application to the Mass-Luminosity Ratio of the Coma Cluster, Astrophys. J., 162, 333CrossRefGoogle Scholar
Ruzmaikin, A., Sokolov, D., & Shukurov, A. 1989, The Dynamo Origin of Magnetic Fields in Galaxy Clusters, MNRAS, 241, 1CrossRefGoogle Scholar
Rybicki, G. B. & Lightman, A. L. 1979, Radiative Processes in Astrophysics (New York: Wiley)Google Scholar
Ryu, D., Kang, H., & Biermann, P. L. 1998, Cosmic Magnetic Fields in Large Scale Filaments and Sheets, Astron. Astrophys., 335, 19Google Scholar
Sarazin, C. L. 1999, The Energy Spectrum of Primary Cosmic-Ray Electrons in Clusters of Galaxies and Inverse Compton Emission, Astrophys. J., 520, 529CrossRefGoogle Scholar
Schlickeiser, R., Sievers, A., & Thielmann, H. 1987, The Diffuse Radio Emission from the Coma Cluster, Astron. Astrophys., 182, 21Google Scholar
Schneider, P., King, L., & Erben, Th. 2000, Cluster Mass Profiles from Weak Lensing: Constraints from Shear and Magnification Information, Astron. Astrophys., 353, 41Google Scholar
Soker, N. 1997, Magnetic Fields and Inflow in Cluster Cooling Flows, in Galactic and Cluster Cooling Flows, ed. Soker, N., ASP Conf. Ser. (San Francisco: Astronomical Society of the Pacific), 115, 182Google Scholar
Stone, J. M. & Norman, M. L. 1992a, ZEUS-2D: A Radiation Magnetohydrodynamics Code for Astrophysical Flows in Two Space Dimensions. I – The Hydrodynamic Algorithms and Tests, Astrophys. J. Suppl., 80, 753CrossRefGoogle Scholar
Stone, J. M. & Norman, M. L. 1992b, ZEUS-2D: A Radiation Magnetohydrodynamics Code for Astrophysical Flows in Two Space Dimensions. II. The Magnetohydrodynamic Algorithms and Tests, Astrophys. J. Suppl., 80, 791CrossRefGoogle Scholar
Sturrock, P. A. & Stern, R. 1980, Is the Galactic Corona Produced by Galactic Flares?, Astrophys. J., 238, 98CrossRefGoogle Scholar
Sunyaev, R. A. & Zel’dovich, Y. B. 1970, The Spectrum of Primordial Radiation, its Distortions and their Significance, Comments Astrophys. Space Phys., 2, 66Google Scholar
Taylor, G. B., Fabian, A. C., & Allen, S. W. 2002, Magnetic Fields in the Centaurus Cluster, MNRAS, 334, 769CrossRefGoogle Scholar
Tribble, P. C. 1993, Radio Haloes, Cluster Mergers, and Cooling Flows, MNRAS, 263, 31Google Scholar
Vallée, J. P., MacLeod, J. M., & Broten, N. W. 1986, A Large-Scale Magnetic Feature in the Galaxy Cluster A 2319, Astron. Astrophys., 156, 386Google Scholar
Vogt, C. & Enßlin, T. A. 2005, A Bayesian View on Faraday Rotation Maps Seeing the Magnetic Power Spectra in Galaxy Clusters, Astron. Astrophys., 434, 67CrossRefGoogle Scholar
Völk, H. J. & Atoyan, A. M. 2000, Early Starbursts and Magnetic Field Generation in Galaxy Cluster, Astrophys. J., 541, 88CrossRefGoogle Scholar
Willson, M. A. G. 1970, Radio Observations of the Cluster of Galaxies in Coma Berenices – the 5C4 Survey, MNRAS, 151, 1CrossRefGoogle Scholar
Xu, H., Li, H., Collins, D. C., Li, S., & Norman, M. L. 2009, Turbulence and Dynamo in Galaxy Cluster Medium: Implications on the Origin of Cluster Magnetic Fields, Astrophys. J., 698, L14CrossRefGoogle Scholar
Xu, H., Li, H., Collins, D. C., Li, S., & Norman, M. L. 2011, Evolution and Distribution of Magnetic Fields from Active Galactic Nuclei in Galaxy Clusters. II. The Effects of Cluster Size and Dynamical State, Astrophys. J., 739, 77CrossRefGoogle Scholar
Xu, Y., Kronberg, P. P., Habib, S., & Dufton, Q. W. 2006, A Faraday Rotation Search for Magnetic Fields in Large-scale Structure, Astrophys. J., 637, 19CrossRefGoogle Scholar
Zel’dovich, Y. B. & Sunyaev, R. A. 1969, The Interaction of Matter and Radiation in a Hot-Model Universe, Astr. Space Sci., 4, 301CrossRefGoogle Scholar
Zwicky, F. 1938, On the Clustering of Nebulae, Pub. Ast. Soc. Pacific, 50, 218CrossRefGoogle Scholar

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