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Fig. 2.


Various models of the MOND velocity dispersion profile of Dragonfly 44 discussed in Sect. 3.2. Top panel: radially anisotropic models. The isotropic model, as in Fig. 1, is shown as a solid line, the externally radial anisotropy model as a dashed line, and the pure radial anisotropy model as a dot-dashed line. Bottom panel: tangentially anisotropic models. Three models for the tangential anisotropy with different stellar masses, as discussed in Sect. 3.2, are shown as solid, dashed, and dash-dotted lines.

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