Title:Dynamic Evolutionary Modelling of Globular Star Clusters

Abstract:
We summarise what has been achieved so far in modelling the evolution of individual old globular star 
clusters in the Milky Way.  Gas, Fokker-Planck, Monte Carlo and N-body models are all contributing to this 
project, conducted by different groups, and have complementary advantages and disadvantages.  Almost 
every object that has been studied by these techniques has revealed some surprises, which we highlight.  
We also touch on prospects for new developments.