Substructure and Gas Clumping in the Outskirts of Abell 133
Galaxy clusters are powerful tools for studying various astrophysical principles. Gas accreting onto the cluster is heated to 10^7-10^8 K through adiabatic compression and shocks, making clusters highly luminous in X-ray imaging. Measurements of the gas density and temperature profiles can be used t...
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| Language: | en |
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2013
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| Online Access: | http://hdl.handle.net/10012/7837 |
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