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1. Full Text THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL'DOVICH-SELECTED GALAXY CLUSTERS AT 0 < z < 1.5
by McDonald, M and Bulbul, E and Haan, T. de and Miller, E. D and Benson, B. A and Bleem, L. E and Brodwin, M and Carlstrom, J. E and Chiu, I and Forman, W. R and Hlavacek-Larrondo, J and Garmire, G. P and Gupta, N and Mohr, J. J and Reichardt, C. L and Saro, A and Stalder, B and Stark, A. A and Vieira, J. D and Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States) and Argonne National Lab. (ANL), Argonne, IL (United States)
The Astrophysical journal, ISSN 0004-637X, 07/2016, Volume 826, Issue 2, pp. 124 - 124
galaxies: clusters: intracluster medium | X-rays: galaxies: clusters | galaxies: clusters: general | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Galactic clusters | Enrichment | X rays | Metallicity | Clusters | X-ray telescopes | Evolution | XMM (spacecraft) | ASTRONOMY AND ASTROPHYSICS
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2. Full Text Constraining Gas Motions in the Intra-Cluster Medium
by Simionescu, Aurora and ZuHone, John and Zhuravleva, Irina and Churazov, Eugene and Gaspari, Massimo and Nagai, Daisuke and Werner, Norbert and Roediger, Elke and Canning, Rebecca and Eckert, Dominique and Gu, Liyi and Paerels, Frits
Space science reviews, ISSN 0038-6308, 3/2019, Volume 215, Issue 2, pp. 1 - 44
Astrophysics and Astroparticles | Planetology | Intracluster medium | Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) | X-ray spectroscopy | Large-scale structure | Aerospace Technology and Astronautics | Physics | Clusters of galaxies | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Viscosity | Emission lines | Turbulence | Turbulent flow | Galaxies | Balances (scales) | Calorimeters | Emission | X-ray emissions | Universe | Velocity | Baryons | Sunyaev-Zeldovich effect | Constraining | Galactic clusters | Surface brightness | Evolution | Variation | Nebulae | Tracers
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3. Full Text HOW AGN JETS HEAT THE INTRACLUSTER MEDIUM-INSIGHTS FROM HYDRODYNAMIC SIMULATIONS
by Karen Yang, H.-Y and Reynolds, Christopher S
The Astrophysical journal, ISSN 0004-637X, 09/2016, Volume 829, Issue 2, p. 90
hydrodynamics | methods: numerical | galaxies: active | galaxies: clusters: intracluster medium | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Turbulent energy | Cold gas | Cooling | Turbulent flow | Accretion | Fluid dynamics | Computer simulation | Galaxies | Computational fluid dynamics | Radiative cooling | Fluid flow | Hydrodynamics | Entropy | Thermal energy | Galactic clusters | Shock heating | Bubbles | Active galactic nuclei | Adiabatic flow | Microprocessors | Cones | Feedback | Cooling flows (astrophysics) | Deposition | HYDRODYNAMIC MODEL | GALAXY CLUSTERS | RADIATIVE COOLING | COMPRESSION | GALACTIC EVOLUTION | PRECESSION | COMPARATIVE EVALUATIONS | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | TURBULENT HEATING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | GALAXIES | SHOCK HEATING | FEEDBACK | GALAXY NUCLEI | ENTROPY
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4. Full Text On the Challenges of Cosmic-Ray Proton Shock Acceleration in the Intracluster Medium
by Wittor, Denis
New astronomy, ISSN 1384-1076, 05/2021, Volume 85, p. 101550
Intracluster medium | Shock waves | Cosmic-ray acceleration | Gamma rays | Analysis | Particle accelerators
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5. Full Text Resolved magnetic dynamo action in the simulated intracluster medium
by Vazza, F and Brunetti, G and Brüggen, M and Bonafede, A
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 2018, Volume 474, Issue 2, pp. 1672 - 1687
Dynamo -MHD- methods: numerical | Galaxies: clusters: intracluster medium | Intergalactic medium | Large-scale structure of Universe | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Coma | Turbulence | Red shift | Turbulent flow | Galaxies | Pollution sources | Computer simulation | Rotation | Galactic clusters | Faraday rotation | Faraday effect | Magnetism | Extragalactic radio sources | Magnetic fields | Spatial resolution | Maxwellian distribution
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6. Full Text SUPPRESSION OF ELECTRON THERMAL CONDUCTION IN THE HIGH β INTRACLUSTER MEDIUM OF GALAXY CLUSTERS
by Roberg-Clark, G. T and Drake, J. F and Reynolds, C. S and Swisdak, M
Astrophysical journal. Letters, ISSN 2041-8205, 10/2016, Volume 830, Issue 1, pp. L9 - L9
plasmas | methods: numerical | turbulence | galaxies: clusters: intracluster medium | conduction | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Galactic clusters | Resonant interactions | Magnetic resonance | Conduction heating | Plasma (physics) | Heat flux | Heat transfer | Whistlers | MAGNETIC FIELDS | DISTRIBUTION | ELECTRONS | GALAXY CLUSTERS | THERMAL CONDUCTION | INTERACTIONS | SIMULATION | HIGH-BETA PLASMA | HEAT | WHISTLERS | DISTRIBUTION FUNCTIONS | THERMODYNAMICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | RESONANCE | MEAN FREE PATH | WHISTLER INSTABILITY | HEAT FLUX | SCATTERING
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7. Full Text Cosmic-Ray Feedback Heating of the Intracluster Medium
by Ruszkowski, Mateusz and Yang, H.-Y. Karen and Reynolds, Christopher S
The Astrophysical journal, ISSN 0004-637X, 07/2017, Volume 844, Issue 1, p. 13
cosmic rays | galaxies: active | galaxies: clusters: intracluster medium | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Computer simulation | Collimation | Cosmic rays | Dispersion | Finite element method | Active galactic nuclei | Star formation | Energy | Feedback | Heating | Thermalization (energy absorption) | Grid refinement (mathematics) | Star & galaxy formation | Cooling flows (astrophysics) | Physics - High Energy Astrophysical Phenomena | DISPERSIONS | INSTABILITY | THERMALIZATION | GALAXY CLUSTERS | LIMITING VALUES | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | ATMOSPHERES | COSMIC RADIATION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | AVAILABILITY | STARS | GALAXIES | HADRONS | FEEDBACK | GALAXY NUCLEI
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