3D Temperature Distribution
High Resolution Picture
(343 KB)
343 KB
(Indeo 5.10)
(~25 MB)
ca. 25 MB
(DivX 4)
(5.8 MB)
5.8 MB
(7.71 MB)
7.71  MB
Temperature dsitributionin a (10 Mpc)^3 cube. The infall of several subclusters onto the cluster centre and the resulting temperature evolution of ICM can be seen. The simulation starts at z=1 and extends to roughly 10 Gyrs into the future.
Institute for Astrophysics, University of Innsbruck