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• W3100470912 abstract "We present a new method for constructing equilibrium phase models for stellar systems, which we call the iterative method. It relies on constrained, or guided evolution, so that the equilibrium solution has a number of desired parameters and/or constraints. This method is very powerful, to a large extent due to its simplicity. It can be used for mass distributions with an arbitrary geometry and a large variety of kinematical constraints. We present several examples illustrating it. Applications of this method include the creation of initial conditions for N-body simulations and the modelling of galaxies from their photometric and kinematic observations." @default.
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• W3100470912 date "2009-01-11" @default.
• W3100470912 modified "2023-10-18" @default.
• W3100470912 title "An iterative method for constructing equilibrium phase models of stellar systems" @default.
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• W3100470912 doi "https://doi.org/10.1111/j.1365-2966.2008.14110.x" @default.
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