Clumpy Substructures in Globular Cluster Tidal Tails

Details Clumpy Substructures in Globular Cluster Tidal Tails Clumpy Substructures in Globular Cluster Tidal Tails

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cemda..91...59d&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, Volume 91, Issue 1-2, pp. 59-73

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Numerical Simulations, Globular Clusters, Computational Astrophysics

Scientific paper

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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