AbstractWe present here new XMM-Newton observations of 3 relatively cool clusters at z≈0.4, complemented by archival observations of 3 other clusters at similar redshift. We derived the M–T and R–T relations from the hydrostatic equation using an isothermal temperature distribution.
Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z0.4
Advances in Space Research ; 42 , 3 ; 576-577
2008-03-11
2 pages
Article (Journal)
Electronic Resource
English
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