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Fig. 15
Dark matter mass fraction of NGC 1316. By considering the dark and luminous components our model separately, we can assess what fraction of the mass at each radius is DM. This plot is made for the model that best fits the kinematic data: β0 = 0.50, Γ = 2.8 M⊙/L⊙, a = 5 kpc, and σDM = 289 km s-1.
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