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Stellar Evolution and Dynamics in Star Clusters
STELLAR EVOLUTION AND DYNAMICS IN STAR CLUSTERS
SIMON F. PORTEGIES ZWART
7
9 Astronomical Institute Anton Pannekoek, Kruislaan 403, NL-1098 SJ Amsterdam
9 CHRISTOPHER A. TOUT
1
Department of Mathematics, Monash University, Clayton, Victoria 3168, Australia.
t
c
O AND
HYUNG MOK LEE
0
2 Dept. of Earth Sciences, Pusan National University, Pusan 609-735, Korea
1
v Abstract. Dynamical models of star clusters are maturing in the sense that effects other than
9
0 simple point particle dynamics are taken into account. We summarize the relevance of and prospects
2 for this new generation of N-body models.
0
1
7
9
/ 1. Summary and Introduction
h
p
- Realistic star clusters are not born instantly nor are they isolated from external perturbations nor
o do they consist of single time-independent equal-mass points. On the contrary a realistic star cluster
r
t is born gradually from a contracting gas cloud, which is embedded in the external potential of a
s
a galaxy, and consists of evolving single stars as well as multiple systems. Owing to lack of computer
: power and partially to lack of software, computations, in which all these effects are accounted for,
v
i have not yet been performed.
X However numerical models of star clusters are beginning to come of age and incorporate devi-
r
a ations from the ideal star cluster. Some models already include mutual interaction between stellar
evolution and star cluster dynamics (see Chernoff Weinberg 1990; Fukushige Heggie 1995;
de la Fuente Marcos 1996; Spurzem Aarseth 1996;
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