Fig. 7 from On Universal Halos and the Radial Orbit Instability

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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. 7.

Phase‐space density of the final halos, ﹩\rho / \sigma ^{3}_{r}﹩ (solid lines), along with their best‐fit slopes (dashed lines). Curves are offset by 1 dex for clarity. Fits are as follows: halo a, ﹩\alpha =-1.32﹩; halo b, ﹩\alpha =-2.04﹩; halo c, ﹩\alpha =-1.49﹩; halo d, ﹩\alpha =-2.15﹩; halo e, ﹩\alpha =-2.04﹩ (not shown).

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