Kinematic properties of gas and stars in 20 disc galaxies

Ionized gas and stellar kinematical parameters have been measured along the major axis of 20 nearby disc galaxies. We discuss the properties of each sample galaxy, distinguishing between those characterized by regular or peculiar kinematics. In early-type disc galaxies, ionized gas tends to rotate faster than stars and to have a lower velocity dispersion (V-g > V-star and sigma (g) < <sigma>(star)), whereas in late-type spirals, gas and stars show almost the same rotation velocities and velocity dispersions (V-g similar or equal to V-star and sigma (g) similar or equal to sigma (star)). Incorporating the early-type disc galaxies studied by Bertola et al. (1995), Fisher (1997) and Corsini et al. (1999), we have compiled a sample of some 40 galaxies for which the major-axis radial profiles of both the stellar and gaseous components have been measured. The value of sigma (star) measured at R-e/4 turns out to be strongly correlated with the galaxy morphological type, while sigma (g) is not and sometimes takes values above the range expected from thermal motions or small-scale turbulence.