Galaxy Cluster Assembly at z = 0.37

Abstract

We present X-ray and spectroscopic confirmation of a cluster assembling from multiple, distinct\r galaxy groups at z = 0.371. Initially detected in the Las Campanas Distant Cluster Survey, the\r structure contains at least four X-ray-detected groups that lie within a maximum projected\r separation of 4 Mpc and within Δ v = 550 km s -1 of one another. Using Chandra imaging and\r wide-field optical spectroscopy, we show that the individual groups lie on the local σ- T relation\r and derive a total mass of M ≥ 5 × 10 14 M ☉ for the entire structure. We demonstrate that the\r groups are gravitationally bound to one another and will merge into a single cluster with about\r one-third or more the mass of Coma. We also find that although the cluster is in the process of\r forming, the individual groups already have a higher fraction of passive members than the field.\r This result indicates that galaxy evolution on group scales is key to developing the early-type\r galaxies that dominate the cluster population by z ~ 0.