Long-term evolution of isolated N-body systems

Abstract We report results of N-body simulations of isolated star clusters, performed up to the point where the clusters are nearly completely dissolved. Our main focus is on the post-collapse evolution of these clusters. We find that, after core collapse, isolated clusters evolve along nearly a sin...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2002-11, Vol.336 (4), p.1069-1081
Hauptverfasser:	Baumgardt, Holger, Hut, Piet, Heggie, Douglas C.
Format:	Artikel
Sprache:	eng
Schlagworte:	celestial mechanics globular clusters: general methods: numerical stellar dynamics
Online-Zugang:	Volltext
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