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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. 12.

Distribution function as a function of j for different values of energy. Top, halo c; middle, halo d; bottom, distribution function recovered from an N‐body realization of an analytic model with ﹩f=f\left(E\right)﹩; that is, with no j dependence. Solid, dashed, dotted, and long‐dashed line types correspond to different energies, in order of increasing binding energy.

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