Fig. 7 from Adaptive Mesh Refinement Simulations of the Ionization Structure and Kinematics of Damped Lyα Systems with Self‐consistent Radiative Transfer

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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. 7.

Cumulative halo mass function at ﹩z=3﹩ for dark matter only, for runs C1 (thick solid line), B1 (thick dashed line), and A1 (thick dotted line). The thin solid line is the analytical mass function from Mo & White (2002).

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