Not exact matches
«If you really want to have a precise mass measurement of the black hole
in a specific galaxy, you'd better use the slightly more cumbersome
velocity dispersion method,» Ferrarese says.
The new method will be invaluable for statistical studies of large numbers of galaxies, says Laura Ferrarese of Rutgers University
in Piscataway, New Jersey, co-discoverer of the
velocity dispersion correlation.
The team accounted for this, and was able to show that the
velocity dispersion or random motion of the RR Lyrae star population was very high relative to the other stars
in the Milky Way's center.
Stars
in a «well ordered» population are all moving coherently, with nearly the same
velocity, whereas stars
in a disordered population have a wider range of
velocities, implying a greater spatial
dispersion.
An elliptical galaxy's luminosity can be found from the
velocity dispersion of the stars
in the central few kiloparsecs of the galaxy.
Sandra Faber and Robert Jackson discovered
in 1976 a simple relation between the spread of
velocities (called the
velocity dispersion) and the luminosity of elliptical galaxies.
A paper, titled «A High Stellar
Velocity Dispersion and ~ 100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44,» describing their findings was published
in the journal Astrophysical Journal Letters on Thursday.
Masses can be determined from the
dispersion in the measured
velocities of individual stellar members of clusters.
Those waves dominate the vertical
velocity field
in the mixed layer (vortex Rossby waves) and below the first hundred meters (near inertial waves) and they are responsible for the differences
in the vertical transport properties under the various forcing fields as quantified by frequency spectra, vertical
velocity profiles and vertical
dispersion of Lagrangian tracers.