Anisotropic Inhomogeneous Riemann S-Ellipsoids in Spheroidal Halos. I. |
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Authors: | M G Abrahamyan |
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Affiliation: | (1) Erevan State University, Armenia |
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Abstract: | The classical Riemann S-ellipsoids are generalized to account for a Ferrers inhomogeneity in the mass distribution, a three-dimensional
anisotropy of the velocity dispersions, and the gravitation of a spheroidal halo. The Ferrers inhomogeneity does not affect
the equilibrium and stability conditions for the ellipsoids, but only changes the numerical coefficients in the equilibrium
parameters. The anisotropy of the velocity dispersions changes both the equilibrium conditions and the criterion for stability
of the ellipsoids, either extending or limiting the region in which the ellipsoids exist. A halo extends this region in all
cases and stabilizes the ellipsoids. The observed of the velocity dispersions of stars in the neighborhood of the sun are
obtained using the inhomgeneous model.
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Translated from Astrofizika, Vol. 48, No. 4, pp. 613–632 (November 2005). |
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Keywords: | Galaxies: halo anisotropy: subsystems of galaxy |
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