Gravitational N-body Simulation of Galactic Clusters

Details Gravitational N-body Simulation of Galactic Clusters Gravitational N-body Simulation of Galactic Clusters

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..oss.d2007b&link_type=abstract

American Physical Society, Joint Spring Meeting Ohio Section of APS and the Southern Ohio Section of AAPT, April 8-9, 2005, abst

Physics

Scientific paper

We have extended a gravitational N-body simulation code that has been used for solar system studies to the scale of stellar clusters. We have used this code to simulate the dynamics of open or galactic stellar clusters that are characterized by a few hundred newly formed stars embedded in the gas and dust cloud from which they formed. We report on the results of simulations that study the stability of the cluster as the remnant cloud is dispersed over the time-scale of a few million years.

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