author={Stephen L. W. McMillan and Simon Portegies Zwart},
  journal={The Astrophysical Journal},
A star cluster in a galactic nucleus sinks toward the galactic center because of dynamical friction. As it spirals inward, the cluster loses mass through stellar evolution, relaxation driven evaporation, and tidal stripping, eventually dissolving in the galactic tidal field. We model the in-spiral of dense young star clusters near the center of our Galaxy to study the extent of the region of parameter space in which the cluster can reach the inner parsec of the Galaxy within a few million years… 

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