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A summary of Joint Discussion 14

Published online by Cambridge University Press:  01 August 2006

Douglas C. Heggie
Douglas C. Heggie*
Affiliation:
School of Mathematics, University of Edinburgh, King's Buildings, Edinburgh EH9 3JZ, UK email: [email protected]
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Abstract

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Modelling rich star clusters is at an exciting time, now that detailed star-by-star modelling of all open star clusters has become possible. We should renew attention to the modelling of globular star clusters, to enable us to exploit the flood of excellent observational data now available. At the same time, new ideas in star cluster astrophysics require us to broaden the realism of our modelling in various directions.

Keywords

methods: n-body simulationsbinaries: generalstars: evolutionpulsars: generalglobular clusters: generalopen clusters and associations: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 448 - 449
Copyright
Copyright © International Astronomical Union 2007

References

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