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Turbulent heating in galaxy clusters brightest in X-rays

Author

Listed:
  • I. Zhuravleva

    (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA
    Stanford University, 382 Via Pueblo Mall, Stanford, California 94305-4060, USA)

  • E. Churazov

    (Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany
    Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow 117997, Russia)

  • A. A. Schekochihin

    (Rudolf Peierls Centre for Theoretical Physics, University of Oxford, 1 Keble Rd, Oxford OX1 3NP, UK
    Merton College, University of Oxford, Merton St, Oxford OX1 4JD, UK)

  • S. W. Allen

    (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA
    Stanford University, 382 Via Pueblo Mall, Stanford, California 94305-4060, USA
    SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA)

  • P. Arévalo

    (Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretana N 1111, Playa Ancha, Valparaíso, Chile
    Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, 306, Santiago 22, Chile)

  • A. C. Fabian

    (Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK)

  • W. R. Forman

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)

  • J. S. Sanders

    (Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany)

  • A. Simionescu

    (Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 252-5210, Japan)

  • R. Sunyaev

    (Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany
    Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow 117997, Russia)

  • A. Vikhlinin

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)

  • N. Werner

    (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA
    Stanford University, 382 Via Pueblo Mall, Stanford, California 94305-4060, USA)

Abstract

Analysis of X-ray data of galaxy clusters shows that turbulent heating of the intracluster medium is sufficient to counteract the radiative energy losses from the medium.

Suggested Citation

  • I. Zhuravleva & E. Churazov & A. A. Schekochihin & S. W. Allen & P. Arévalo & A. C. Fabian & W. R. Forman & J. S. Sanders & A. Simionescu & R. Sunyaev & A. Vikhlinin & N. Werner, 2014. "Turbulent heating in galaxy clusters brightest in X-rays," Nature, Nature, vol. 515(7525), pages 85-87, November.
  • Handle: RePEc:nat:nature:v:515:y:2014:i:7525:d:10.1038_nature13830
    DOI: 10.1038/nature13830
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