All Tables

Table 1: Comparison of $v_{\rm max}$ [km s^-1] (maximum velocity of rotation curves) and $HW20M_{\rm HI}$ [km s^-1] (Half of the HI profile between points where the intensity falls to 20% of the highest channels in each half of the profile and corrected for relativistic effects; Note: average only with the galaxies which have this datum available) for spiral galaxies in Mathewson et al. (1992) catalogue in barred and non-barred cases as a function of the galaxy type.
Table 2: Comparison of OW3 [km s^-1] (measured velocity width in optical profiles with corrections for the shape of the rotation curve, cosmological stretch and converted to edge-on viewing measured at twice the scale length), RW2 [km s^-1] (measured 21 cm line profile velocity corrected and converted to edge on viewing; Note: average only with the galaxies which have this datum available), M/L [solar units] (corrected mass to light [I-band] ratio; Note: average only with the galaxies which have this datum available) for spiral galaxies in Vogt et al. (2004) catalogue in barred and non-barred cases as a function of the galaxy type. There are no barred galaxies with available data in this catalogue of types +6 or later.
Table 3: Same as Table 2 but only with galaxies considered bona fide members of a cluster of galaxies. There is only one barred galaxy of type +4 "in a cluster'' of Vogt et al. (2004) catalogue, which is not included.