Simulating Astro-E2 Observations of Galaxy Clusters: The Case of Turbulent Cores Affected by Tsunamis
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference23 articles.
1. [ITAL]Chandra[/ITAL] Observation of the Radio Source/X-Ray Gas Interaction in the Cooling Flow Cluster Abell 2052
2. Hot bubbles from active galactic nuclei as a heat source in cooling-flow clusters
3. Cooling flows as a calorimeter of active galactic nucleus mechanical power
4. Characterization of the Astro-E2 X-ray spectrometer
5. Formation and evolution of X-ray clusters - A hydrodynamic simulation of the intracluster medium
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1. Non-steady heating of cool cores of galaxy clusters by ubiquitous turbulence and AGN;Monthly Notices of the Royal Astronomical Society;2020-04-24
2. Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy;Publications of the Astronomical Society of Japan;2018-04-27
3. SIMULATINGASTRO-HOBSERVATIONS OF SLOSHING GAS MOTIONS IN THE CORES OF GALAXY CLUSTERS;The Astrophysical Journal;2016-04-01
4. STABLE HEATING OF CLUSTER COOLING FLOWS BY COSMIC-RAY STREAMING;The Astrophysical Journal;2011-08-25
5. Suzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool Core Clusters;Publications of the Astronomical Society of Japan;2008-10-25
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