We have analyzed XMM-Newton archive data for five clusters of galaxies (redshifts 0.223-0.313) covering a wide range of dynamical states, from relaxed objects to clusters undergoing several mergers. We present here temperature maps of the X-ray gas together with a preliminary interpretation of the formation history of these clusters. © 2007 COSPAR.
CITATION STYLE
Durret, F., & Lima Neto, G. B. (2008). XMM-Newton temperature maps for five intermediate redshift clusters of galaxies. Advances in Space Research, 42(3), 578–580. https://doi.org/10.1016/j.asr.2007.07.033
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