A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z = 0.975

Authors :: Fassbender, R.
Böhringer, H.
Santos, J. S.
Pratt, G. W.
Šuhada, R.
Kohnert, J.
Lerchster, M.
Rovilos, E.
Pierini, D.
Chon, G.
Schwope, A. D.
Lamer, G.
Mühlegger, M.
Rosati, P.
Quintana, H.
Nastasi, A.
de Hoon, A.
Seitz, S.
Mohr, J. J.
Source :: Astronomy and Astrophysics; March 2011, Vol. 527 Issue: 1
Publication Year :: 2011
Abstract: Context.Observations of the formation and evolution of massive galaxy clusters and their matter components provide crucial constraints on cosmic structure formation, the thermal history of the intracluster medium (ICM), galaxy evolution, transformation processes, and gravitational and hydrodynamic interaction physics of the subcomponents.