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• W2078426761 abstract "We find a numerical self-consistent stellar model by finding the distribution function of a thin disk that satisfies simultaneously the Fokker-Planck and Poisson equations. The solution of the Fokker-Planck equation is found by a direct numerical solver using finite differences and a variation of Stone's method. The collision term in the Fokker-Planck equation is found using the local approximation and the Rosenbluth potentials. The resulting diffusion coefficients are explicitly evaluated using a Maxwellian distribution for the field stars. As a paradigmatic example, we apply the numerical formalism to find the distribution function of a Kuzmin-Toomre thin disk. This example is studied in some detail showing that the method applies to a large family of actual galaxies." @default.
• W2078426761 created "2016-06-24" @default.
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• W2078426761 date "2005-10-14" @default.
• W2078426761 modified "2023-10-02" @default.
• W2078426761 title "Numerical self-consistent stellar models of thin disks" @default.
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• W2078426761 doi "https://doi.org/10.1051/0004-6361:20053176" @default.
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