Realistic N - Body Simulations of Globular Clusters

  • A. Dougal Mackey
Part of the Lecture Notes in Physics book series (LNP, volume 760)

This chapter is an introduction to realistic N-body modelling of globular clusters – specifically, why it might be desired to conduct such models and what constitutes their key ingredients. Detailed consideration is also given to the analysis of data from such simulations, and how it is increasingly becoming more important to perform simulated observations in order to derive quantities that are directly comparable with real-world measurements. The most salient points from this general discussion are illustrated via an extensive case study concerning N-body modelling of massive stellar clusters in the Large and Small Magellanic Clouds.


Black Hole Globular Cluster Star Cluster Initial Mass Function Magellanic Cloud 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer-Verlag Berlin Heidelberg 2008

Authors and Affiliations

  • A. Dougal Mackey
    • 1
  1. 1.Institute for AstronomyUniversity of Edinburgh Royal ObservatoryBlackford HillUK

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