X-Ray Nature of Abell Sources Super Galaxy Clusters

One of the reasons of this study is to find an answer to the question of how affect galaxy cluster environments and intergalactic activities of evolution of member galaxies. For this purpose, six nearby (z<0.14) galaxy clusters (A1644, A1736, A3528, A3558, A3562, A3571) have been selected from XMM-Newton archive in order to determine X-ray properties of galaxies which in clusters and to compare galaxies belong to a cluster with galaxies do not belong to any cluster where any field. Selected galaxy clusters are newly forming clusters (proto galaxy clusters), their intra cluster medium (ICM) hasn't formed completely and thus individual sources (galaxies) well stand out particularly. The other reason of this study is to find out global spectral properties of selected clusters.