This could be a direct consequence of the high internal velocity dispersion in the molecular clouds.

In this case the velocity dispersion of its stars is not related to its mass.

At large radii, radial velocity dispersion exhibit strange behavior.

Using the velocity dispersion, the cluster mass has been estimated to 10 solar masses.

Here the velocity dispersion is much smaller.

In both families, the tangential velocity dispersion undergoes a jump as increases past .

The velocity dispersion of material around it is measured to be 160 km/s.

When a wave propagates through subsurface materials both energy dissipation and velocity dispersion takes place.

More luminous elliptical galaxies have larger central velocity dispersions.

Groups and clusters of galaxies have a wider range of velocity dispersions than smaller objects.