Galaxies and star clusters are collisionless self- gravitating
systems. The models of their equilibrium states are solutions of
the corresponding equations based on equations of motion of the
particles of which the system consists. Therefore, modeling these
systems requires solution of a series of problems, starting from
the one-body problem. In this book models of various
axially-symmetric collisionless systems are built, among which
there are thin disk, bulge of a spiral galaxy and prolate galaxy in
equilibrium and evolutionary states.
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