Fig. 11.
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Mass models for a FDM halo. The top panel is Case 1, when M200 is completely free (and the cosmological baryon fraction is not obeyed), while the bottom panel is Case 2, imposing a lower bound in M200, min. Curves are as in Figure 9. The black triangles indicate the position of rt, the transition radius between the soliton and the NFW halo.
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