Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap.....49..306a&link_type=abstract
Astrophysics, Volume 49, Issue 3, pp.306-319
Astronomy and Astrophysics
Astrophysics
Galaxies, Halo, Anisotropy
Scientific paper
Classical S-type Riemann ellipsoids are generalized taking a Ferrers-type inhomogeneity in the mass distribution, a three-dimensional anisotropy in the dispersion in the velocities, and the gravitation of a spherical halo into account. A Ferrers inhomogeneity in the mass distribution does not affect the equilibrium conditions for the ellipsoids, but only changes the numerical coefficients in the equilibrium parameters. An anisotropy in the dispersion in the velocities does change the equilibrium conditions, expanding or contracting the region in which embedded ellipsoids exist. A halo extends this region in all cases.
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