Table 1.
Properties of the sample galaxies (see Iorio et al. 2017 for details).
| Galaxy | D | log(SFR) | ⟨Vc⟩ | ⟨i⟩ | ⟨PA⟩ | M200 | c | n | M⋆ | R⋆ | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (Mpc) | (M⊙ yr−1) | (km s−1) | (°) | (°) | (1010 M⊙) | (107 M⊙) | (kpc) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | ||
| WLM | 1.0 | −2.13 ± 0.08 | 38.7 ± 3.4 | 74.0 ± 2.3 | 174.0 ± 3.1 |
 |
17 | 0.887 | 1.62 | 0.75 | |
| DDO 52 | 10.3 | −1.82 ± 0.08 | 51.1 ± 6.3 | 55.1 ± 2.9 | 6.5 ± 2.0 |
 |
17.3 | 0.894 | 5.27 | 0.94 | |
| DDO 87 | 7.4 | −1.95 ± 0.07 | 50.3 ± 9.1 | 42.7 ± 7.3 | 238.6 ± 4.7 |
 |
17.6 | 0.900 | 3.3 | 1.13 | |
| NGC 2366 | 3.4 | −0.97 ± 0.07 | 57.7 ± 5.4 | 65.1 ± 4.2 | 39.8 ± 2.8 |
 |
17.3 | 0.894 | 6.95 | 1.54 | |
| DDO 126 | 4.9 | −1.80 ± 0.06 | 38.6 ± 3.1 | 62.2 ± 2.9 | 140.7 ± 3.5 |
 |
20.6 | 0.947 | 1.61 | 0.82 | |
| DDO 168 | 4.3 | −1.67 ± 0.06 | 56.2 ± 6.9 | 62.0 ± 2.6 | 272.7 ± 4.2 |
 |
16.8 | 0.883 | 5.9 | 0.82 | |
| DDO 133 | 3.5 | −1.91 ± 0.05 | 47.2 ± 5.1 | 38.9 ± 3.7 | −3.8 ± 8.9 |
 |
25.8 | 0.984 | 3.04 | 0.804 | |
| DDO 50 | 3.4 | −0.95 ± 0.04 | 38.7 ± 10.1 | 33.1 ± 4.6 | 174.9 ± 5.9 |
 |
26.2 | 0.985 | 10.72 | 0.89 | |
| DDO 47 | 5.2 | −1.61 ± 0.04 | 62.6 ± 5.2 | 37.4 ± 1.7 | 317.4 ± 7.3 |
 |
20.5 | 0.946 | 9.4 | 0.7 | |
| DDO 101 | 6.4 | −2.45 ± 0.09 | 52.9 ± 3.6 | 52.4 ± 1.7 | 287.4 ± 3.6 |
 |
28.9 | 0.993 | 6.54 | 0.58 |
Notes. (1) Distance; (2) integrated SFR from FUV (see Sect. 3.2); (3) mean circular velocity (i.e. asymmetric-drift corrected) of the outer HI disc; (4) HI disc inclination; (5) HI disc position angle. Parameters of the best-fit model for the core-NFW halo and the stellar disc from Read et al. (2017): (6) DM mass within R200; (7) DM halo concentration; (8) index of the DM halo core function; (9) stellar mass; (10) stellar disc scale lenght.
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