Journal
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
Volume 91, Issue 1-2, Pages 59-73Publisher
SPRINGER
DOI: 10.1007/s10569-005-3221-y
Keywords
numerical simulations; globular clusters; computational astrophysics
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In this paper, we present some preliminary results of numerical simulations of a globular cluster orbiting in the inner region of a triaxial galaxy. The formation and evolution of tidal tails around the cluster is discussed, together with their morphology, which shows clumpy substructures as observed, for example, in the galactic globular cluster Palomar 5.
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