X-Ray Clusters

The following visualization is of 1015 solar mass cluster showing a region of comoving size approximately 10 Mpc on a side.  It was performed with the Enzo AMR code and is described in more detail in this paper.

1. Gas density evolution
   

2. Dark matter evolution
   

3. HI (cold gas) evolution
   

4. Metallicity evolution
   

5. Stellar density evolution