Astrophysics (index)about

velocity dispersion

(σ, dispersion)
(statistical dispersion of velocities of a group of objects)

A velocity dispersion (σ) is the statistical dispersion of velocities of a group of objects about the mean velocity. It is a quality of interest in open clusters, globular clusters, galaxies, galaxy clusters, and superclusters. Radial velocity can be determined by Doppler shift and the width of the effected spectral lines can determine dispersion across a group, which, with the virial theorem, can determine the group's mass.

Statistical dispersion characterizes the "spread". The standard deviation of a sample set is one measure of statistical dispersion.

The term dispersion (or chromatic dispersion) is also used in optics and spectroscopy (or any type of wave such as sound waves) to indicate waves' differences in velocity through a medium when the velocity depends upon the frequency. This is used by refractive spectroscopes and also is the source of chromatic aberration in lenses.


Referenced by:
broad emission line region
Faber-Jackson relation (FJR)
fast radio burst (FRB)
fundamental plane
protoplanetary disk (PPD)
Seyfert galaxy
velocity-metallicity relation
virial parameter
virial theorem