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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. 3.

Density profiles of each of the final halos at ﹩z=0﹩ (solid lines). Also shown (dashed lines) are the best‐fit NFW density profiles for halos b, d, and e and power‐law fits for halos a and c.

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