  We consider global HI and optical properties of about three hundred nearby
galaxies with V$_0 < 500$ km/s. The majority of them have individual
photometric distance estimates. The galaxy sample parameters, e.g. their linear
diameters, their HI mass-to-luminosity ratio, their total mass-to-luminosity
ratio, their mean optical surface brightness show some known and some new
correlations implying a meaningful dynamic explanation. For the LV galaxies
their HI mass and angular momentum follow a nearly linear relation expected for
rotating gaseous disks being near the threashold of gravitational instability,
favourable for active star formation.
