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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. 2.

Amplitude of the assumed fiducial UVB at 13.6 eV in standard units of 10−21 ergs s−1 cm−2 sr−1 Hz−1. Shown are the quasar (dashed line) component ﹩I_{21,q}﹩, the stellar (dotted line) component ﹩I_{21,*}﹩, and their sum (solid line) at the hydrogen Lyman edge for ﹩\beta _{*}=\beta _{q}=1﹩. For comparison we also plotted the total UVB from Abel & Haehnelt (1999; dash‐dotted line).

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