XMM-Newton temperature maps for five intermediate redshift clusters of galaxies
arXiv:0707.4120 · doi:10.1016/j.asr.2007.07.033
Abstract
We have analyzed XMM-Newton archive data for five clusters of galaxies (redshifts 0.223 to 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.
4 pages, 2 figs. Accepted for publication in the Proceedings of the 36th COSPAR Scientific Assembly
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Cited by in corpus (5)
- Thermo-dynamic and chemical properties of the Intra-Cluster Medium
- Simulations of the merging galaxy cluster Abell 3376
- Spiral-like structure in nearby clusters of galaxies
- On the influence of non-thermal pressure on the mass determination of galaxy clusters
- Detection of X-ray galaxy clusters based on the Kolmogorov method