Research Article

Vortex Structures in a Rotating BEC Dark Matter Component

Figure 3

Rotation curves for NGC1560 ( 5 . 0 , 2 . 1 5 , 0 . 5 , 5 . 0 , 1 . 0 ), NGC753 ( 5 . 0 , 2 . 0 0 , 3 . 0 , 6 . 5 , 1 . 0 ), NGC801 ( 5 . 0 , 2 . 1 5 , 3 . 0 , 6 . 5 , 1 . 0 ), and NGC3198 ( 5 . 0 , 2 . 0 0 , 1 . 2 , 6 . 5 , 2 . 0 ) compared to model calculations. The plot assignments are as in Figure 2. The parentheses give the parameters used in the format ( 𝑟 0 , 𝛾 , 𝑏 , 𝐿 𝑣 , 𝑑 ). Notice the change of radial distance scale for NGC1560.
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