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Table 1.

Summary of the main parameters of the sample.

Galaxy Type i d M MHI Qbar Lbar PAbar ϵbar
(deg) (Mpc) (1010M) (1010M) (arcsec) (deg)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
IC 1438 24 33.8 3.1 0.12 0.178 23.8 121.0 0.51
NGC 4303 34 16.5 7.2 0.45 0.535 36.1 178.0 0.69
NGC 4371 (L)SBa(r, bl, nr)00/+ 59 16.8 3.2 0.08 0.234 34.8 ( ⋆ ) 159.0 ( ⋆ ) 0.51 ( ⋆ )
NGC 4643 44 25.7 10.7 0.03 0.272 49.9 133.0 0.47
NGC 4981 54 24.7 2.8 0.35 0.093 18.9 147.0 0.57
NGC 4984 (R′R)SABa(l, bl, nl)0/a 53 21.3 4.9 0.03 0.176 30.0 94.0 0.30
NGC 5248 (R′)SAB(s, nr)bc 41 16.9 4.7 0.40 0.138 27.4 128.0 0.36
NGC 6902 37 38.5 6.4 2.34 0.045 16.2 132.5 0.36
NGC 7755 52 31.5 4.0 0.65 0.401 24.6 125.0 0.56

Notes. Columns (1)−(6) are extracted from Table 1 in Paper I. For details, we refer to that paper. (1) Galaxy name; (2) morphological type by Buta et al. (2015); (3) inclination of the galaxy; (4) distance to the galaxy; (5) total stellar mass; (6) total H I mass; (7) bar maximum gravitational torque from Díaz-García et al. (2016). Columns (8)−(10) are taken from Herrera-Endoqui et al. (2015) with the exception of NGC 4371, which was found to be inaccurate and taken from Gadotti et al. (2015) instead: (8) bar length; (9) position angle of the bar; (10) ellipticity of the bar.

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