Spherically Symmetric Stellar Clusters with Anisotropy And Cutoff Energy in Momentum Distribution. I. The Newtonian Regime

Astronomy and Astrophysics – Astronomy

Scientific paper

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Dense Matter, Galaxies: Star Clusters, Hydrodynamics

Scientific paper

We construct numerical models of spherically symmetric Newtonian stellar
clusters with anisotropic distribution functions. These models
generalize solutions obtained earlier for isotropic Maxwellian
distribution functions with an energy cutoff and take into account
distributions with different levels of anisotropy.

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