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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. 4.

Top: Upper four solid lines show the H I column density frequency distribution ﹩f( N,X) ﹩ for runs C−1, C0, C1, and C2 (from thinnest to thickest line), all at ﹩z=3﹩. The lower two lines are the Γ function fits to the SDSS DLA survey data from Prochaska et al. (2005) for ﹩z=2.5{\mbox{--}} 3.0﹩ (dashed line) and ﹩z=3.0{\mbox{--}} 3.5﹩ (dotted line). Bottom: Same as top, except that the upper three lines give ﹩f( N,X) ﹩ for runs C1 (solid line), B1 (dashed line), and A1 (dotted line).

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