Professor of Astronomy

Columbia University

Greg Bryan

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. Bullet Gas density evolution

  2. Bullet Dark matter evolution

  3. Bullet HI (cold gas) evolution

  4. Bullet Metallicity evolution

  5. Bullet Stellar density evolution