Multi-fluid shocks in clusters of galaxies: Entropy, σv–T, M–T and LX–T scalings
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
Reference57 articles.
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2. Clusters and cosmology;Bahcall;Phys. Rep.,2000
3. Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed;Bell;MNRAS,2001
4. Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays;Bell;MNRAS,2004
5. Clusters of galaxies as storage room for cosmic rays;Berezinsky;Astrophys. J.,1997
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1. Collisionless Shocks in Partly Ionized Plasma with Cosmic Rays: Microphysics of Non-thermal Components;Space Science Reviews;2013-05-09
2. ENTROPY AT THE OUTSKIRTS OF GALAXY CLUSTERS AS IMPLICATIONS FOR COSMOLOGICAL COSMIC-RAY ACCELERATION;The Astrophysical Journal;2013-03-21
3. Collisionless Shocks in Partly Ionized Plasma with Cosmic Rays: Microphysics of Non-thermal Components;Microphysics of Cosmic Plasmas;2013
4. Magnetic Fields, Relativistic Particles, and Shock Waves in Cluster Outskirts;Space Science Reviews;2011-06-09
5. EFFECTS OF NEUTRAL HYDROGEN ON COSMIC-RAY PRECURSORS IN SUPERNOVA REMNANT SHOCK WAVES;The Astrophysical Journal;2011-03-18
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