Rossi X‐Ray Timing ExplorerSpectrum of A2319
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/565/i=2/a=877/pdf
Reference33 articles.
1. Inverse Compton Scattering as the Source of Diffuse Extreme‐Ultraviolet Emission in the Coma Cluster of Galaxies
2. Extreme‐Ultraviolet Emission in Abell 1795, Abell 2199, and the Coma Cluster
3. A New Radio–X-Ray Probe of Galaxy Cluster Magnetic Fields
4. 26.3 MHz radio source survey. III - Correlation with extragalactic X-ray sources
5. The radio and X-ray properties of Abell 2319
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1. Possible non-thermal origin of the hard X-ray emission in the merging galaxy cluster SPT-CL J2031−4037;Monthly Notices of the Royal Astronomical Society;2022-08-29
2. Suzaku Observation of the Radio Halo Cluster Abell 2319: Gas Dynamics and Hard X-Ray Properties;Publications of the Astronomical Society of Japan;2009-12-25
3. Chandrameasurements of non-thermal-like X-ray emission from massive, merging, radio halo clusters;Monthly Notices of the Royal Astronomical Society;2009-11-01
4. GALAXY CLUSTERS IN THESWIFT/BURST ALERT TELESCOPE ERA: HARD X-RAYS IN THE INTRACLUSTER MEDIUM;The Astrophysical Journal;2008-12-01
5. Heating and Acceleration of Intracluster Medium Electrons by Turbulence;The Astrophysical Journal;2008-07-20
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