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

Table 4

The best rotation curve data fit BEC + baryonic and NFW + baryonic parameters for the dwarf galaxy sample.

Galaxy	(BEC)	(BEC)			(BEC)	(NFW)	(NFW)			(NFW)	1
	kpc		kg/m^3	kpc		kpc		kg/m^3	kpc
IC 2574	1.2	0.1122	0.4	13	68.47	7.9	28.44	0	0	714.73	44.74
HoI	0.2	0.0107	3.6	1.9	95.26	0.9	0.533	0	0	241.30	20.27
HoII	1.2	0.4431	0.2	7.69	33.33	1.7	0.642	4	92	43.86	26.72
DDO 39	1.3	1.1235	0.7	10.01	69.39	4.3	7.21	43	35	69.82	17.02
DDO 53	0.2	0.0061	1.8	2.5	20.05	1.6	0.976	1	24	51.53	10.42
DDO 154	3.1	3.3502	0.2	5.8	1.48	3.2	4.52	0	0	9.40	9.30
M81dwB nor	0.9	1.023	3.7	0.7	6.19	0.7	0.705	0	0	8.4	10.42