Research Article

Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves

Figure 6

The density parameter of the BEC model is shown as function of in (a), and the density parameter of the NFW model is shown as function of in (b). The HSB, LSB, and dwarf galaxies are represented by filled circles, empty triangles, and filled triangles, respectively.
(a)
(b)