Kinematic Properties of Anisotropic Models of Spherical Galaxies

Details Kinematic Properties of Anisotropic Models of Spherical Galaxies Kinematic Properties of Anisotropic Models of Spherical Galaxies

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..783h&link_type=abstract

Astronomy and Astrophysics, Vol. 283, NO. 3/MAR(III), P. 783, 1994

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

The energy-angular momentum distribution, the line-of-sight velocity dispersion and the line-of-sight velocity distribution for a class of anisotropic models of spherical galaxies are studied. All the distribution functions used are constructed in such a way as to give the same density profile, which is a good approximation to the Vaucouleurs law. The results show that the models distribution functions used have kinematic properties that are in principle close to those of real galaxies.

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