Image Details

Choose export citation format:

Adaptive Mesh Refinement Simulations of the Ionization Structure and Kinematics of Damped Lyα Systems with Self‐consistent Radiative Transfer

  • Authors: Alexei O. Razoumov, Michael L. Norman, Jason X. Prochaska, and Arthur M. Wolfe

Razoumov et al. 2006 The Astrophysical Journal 645 55.

  • Provider: AAS Journals

Caption: Fig. 3.

I column density in a volume ﹩8\ h^{-1}\ \mathrm{Mpc}\,﹩ on a side and ﹩8\ h^{-1}\ \mathrm{Mpc}\,﹩ thick (comoving), from run C1 at ﹩z=3﹩. The insets are ﹩600\ h^{-1}\ \mathrm{kpc}\,﹩ (top) and ﹩80\ h^{-1}\ \mathrm{kpc}\,﹩ (bottom) on a side in comoving units, translating into an approximately 10 kpc (physical units) DLA around the disk galaxy in the center of the bottom panel. The DLA column densities correspond to green and up in the color map on the right. The resolved dynamic range in this model is 8192.

Other Images in This Article
Copyright and Terms & Conditions