Simulations of Spheroidal Systems with Substructure: Trees in Fields
arXiv:astro-ph/9702077 · doi:10.1046/j.1365-8711.1998.01325.x
Abstract
We present a hybrid technique of N-body simulation to deal with collisionless stellar systems having an inhomogeneous global structure. We combine a treecode and a self-consistent field code such that each of the codes model a different component of the system being investigated. The treecode is suited to treatment of dynamically cold or clumpy systems which may undergo significant evolution within a dynamically hot system. The hot system is appropriately evolved by the self-consistent field code. This combined code is particularly suited to a number of problems in galactic dynamics. Applications of the code to these problems are briefly discussed.
13 pages, LaTeX, 13 figures, submitted to MNRAS
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