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On Universal Halos and the Radial Orbit Instability

  • Authors: Joseph D. MacMillan, Lawrence M. Widrow, and Richard N. Henriksen

MacMillan, Widrow, & Henriksen 2006 The Astrophysical Journal 653 43.

  • Provider: AAS Journals

Caption: Fig. 4.

Top: Density profile of halo d at early (﹩z=1.72﹩, dashed line) and late (﹩z=0﹩, solid line) times. The former is offset by 1 dex. Arrows indicate the NFW scale length rs. Bottom: Concentration parameter of the NFW fit to density profiles for the halos as they evolve in time. The solid line represents halo b, the dashed line represents halo d, and the dotted line represents halo e.

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