A study of the velocity distribution for a particular case of the spherical symmetry.

Details A study of the velocity distribution for a particular case of the spherical symmetry. A study of the velocity distribution for a particular case of the spherical symmetry.

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991bobeo.144....1n&link_type=abstract

Bulletin Astronomique de Belgrade, No. 144, p. 1 - 3

Astronomy and Astrophysics

Astronomy

Stellar Systems: Velocity Distribution

Scientific paper

A particular case of spherically symmetric stellar systems, characterised by the mass distribution of the type (1-r2/rl2), is studied. It is obtained that, if the mean radial velocity square varies in the same way as the density, then anisotropic velocity distributions with the transverse component prevailing take place. The fraction of the radial component in the total kinetic energy is not high, even in the case of a very high mean radial-velocity square at the centre it is less than 50%.

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