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Table 2.

Parametric mass models for DM and stellar components of the sample galaxies.

Galaxy Dark matter halo
Stellar disc
Bulge
Type cρDM, 0 V200rc Σ⋆, 0 R z ρb, 0 rb
(const – 106M kpc−3) ( km s−1 – kpc) (106M kpc−2) (kpc) (kpc) (1010M kpc−3) (kpc)
(1) (2) (3) (4) (5) (6) (7) (8)
DDO 154 ISO 28.5 1.32 5.7 0.72 0.144 0 0
IC 2574 ISO 5.0 6.18 14.5 2.85 0.57 0 0
NGC 0925 ISO 6.5 8.90 68.6 4.1 0.82 0 0
NGC 2403 ISO 144.4 1.50 176.4 1.81 0.362 0 0
NGC 2841 NFW 24.8 172.6 684.4 4.2 0.84 1.24 0.394
NGC 2976 ISO 42.8 2.60 247.4 0.9 0.18 0 0
NGC 3198 ISO 45.2 2.80 302.3 3.06 0.612 0 0
NGC 4736 NFW 108.3 40.9 529.8 1.99 0.398 5.3 0.144
NGC 5055 ISO 11.1 7.15 1179.0 3.2 0.64 3.0 0.19
NGC 6946 ISO 31.4 4.80 752.2 2.97 0.594 21.0 0.08
NGC 7331 NFW 9.3 171.2 1160.9 3.3 0.66 10.8 0.175
NGC 7793 ISO 93.5 1.95 420.7 1.3 0.26 0 0

Notes. DM halo profile: (1) type, ISO = isothermal, NFW = Navarro–Frenk–White; (2) concentration or central density; and (3) V200 or core radius. Stellar disc: (4) central surface density Σ⋆, 0 = ρ⋆, 0/(2R); (5) scale radius; and (6) scale height. Bulge (as exponential sphere): (7) central density and (8) scale radius.

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