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Structures and Components in Galaxy Clusters: Observations and Models

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Book cover Multi-scale Structure Formation and Dynamics in Cosmic Plasmas

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 51))

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Abstract

Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. Bubbles of relativistic plasma which are inflated by supermassive black holes of AGNs, cooling and heating of the gas, large scale plasma shocks, cold fronts, non-thermal halos and relics are observed in clusters. These constituents are reflecting both the formation history and the dynamical properties of clusters of galaxies. We discuss X-ray spectroscopy as a tool to study the metal enrichment in clusters and fine spectroscopy of Fe X-ray lines as a powerful diagnostics of both the turbulent plasma motions and the energetics of the non-thermal electron populations. The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters.

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Authors and Affiliations

  1. A.F. Ioffe Institute for Physics and Technology, 194021, St. Petersburg, Russia

    A. M. Bykov

  2. St. Petersburg State Politecnical University, St. Petersburg, Russia

    A. M. Bykov

  3. International Space Science Institute, Bern, Switzerland

    A. M. Bykov

  4. Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85741, Garching, Germany

    E. M. Churazov

  5. Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow, 117997, Russia

    E. M. Churazov

  6. Laboratoire Lagrange, UMR7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Boulevard de l’Observatoire, 06300, Nice, France

    C. Ferrari

  7. Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA, 02138, USA

    W. R. Forman

  8. SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, Netherlands

    J. S. Kaastra & J. de Plaa

  9. Argelander-Institut für Astronomie, University of Bonn, Bonn, Germany

    U. Klein

  10. Astrophysics Science Division, NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA

    M. Markevitch

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  1. A. M. Bykov
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  2. E. M. Churazov
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  3. C. Ferrari
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  4. W. R. Forman
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  5. J. S. Kaastra
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  6. U. Klein
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  7. M. Markevitch
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  8. J. de Plaa
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Correspondence to A. M. Bykov .

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Editors and Affiliations

  1. Dept of Physics Blackett Laboratory, Imperial College London, London, United Kingdom

    Andre Balogh

  2. Ioffe Institute, St. Petersburg, Russia

    Andrei Bykov

  3. Dept of Physics Blackett Laboratory, Imperial College London, London, United Kingdom

    Jonathan Eastwood

  4. SRON Netherlands Institute for Space Res, Utrecht, Utrecht, The Netherlands

    Jelle Kaastra

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Bykov, A.M. et al. (2016). Structures and Components in Galaxy Clusters: Observations and Models. In: Balogh, A., Bykov, A., Eastwood, J., Kaastra, J. (eds) Multi-scale Structure Formation and Dynamics in Cosmic Plasmas. Space Sciences Series of ISSI, vol 51. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-3547-5_5

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