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Fig. 5.


Best-fit rotational curves of the dwarf galaxy sample. The dots with error-bars denote the observed rotational velocity curves. The fitted model, composed by a baryonic and a srBEC component is represented by the black curve. The red short-dashed curve draws the contribution of the stellar component, the blue tiny-dashed curve shows the contribution of the gas, and the long-dashed purple curve denotes the contribution of the srBEC-type DM halo to the rotation curve–models.

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