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- W2070697938 abstract "We study a new class of equilibrium two-parametric distribution functions of spherical stellar systems with a radially anisotropic velocity distribution of stars. The models are less singular counterparts of the so-called generalized polytropes, widely used in the past in works on equilibrium and the stability of gravitating systems. The offered models, unlike the generalized polytropes, have finite density and potential in the centre. The absence of the singularity is necessary for proper consideration of the instability of the radial orbit, which is the most important instability in spherical stellar systems. We provide a comparison of the main observed parameters (i.e. potential, density, anisotropy) predicted by the present models and by other popular equilibrium models." @default.
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- W2070697938 date "2013-08-03" @default.
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- W2070697938 title "Equilibrium models of radially anisotropic spherical stellar systems with softened central potentials" @default.
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- W2070697938 doi "https://doi.org/10.1093/mnras/stt1236" @default.
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