Non-linear models of non-stationary self-gravitating systems and their stability problem
С. Н. НуритдиновAstronomy Department , Tashkent University , Uzbekistan
ABI
Abstract
Abstract Simple analytical non-linear models of non-stationary galaxies are constructed. Their forms are spherical or disk-like. Their radius is Where Here λ is the pulsation amplitude, and (2T/|μ|)0 is the initial virial ratio If λ = 1, then the orbits are purely radial.
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