Turbulent heating in galaxy clusters brightest in X-rays

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 and N. Werner
Additional contact information
I. Zhuravleva: Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA
E. Churazov: Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany
A. A. Schekochihin: Rudolf Peierls Centre for Theoretical Physics, University of Oxford, 1 Keble Rd, Oxford OX1 3NP, UK
S. W. Allen: Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA
P. Arévalo: Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretana N 1111, Playa Ancha, Valparaíso, 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
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

Nature, 2014, vol. 515, issue 7525, 85-87

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.

Date: 2014
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DOI: 10.1038/nature13830

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