ForumSpringerAstron. Astrophys.
ForumWhats NewSearchOrders

Astron. Astrophys. 328, 130-142

Table of Contents
Available formats: HTML | PDF | (gzipped) PostScript

Star cluster ecology

I. A cluster core with encounters between single stars

Simon F. Portegies Zwart1, 2, Piet Hut3, and Frank Verbunt1

1 Astronomical Institute, Postbus 80000, 3508 TA Utrecht, The Netherlands
2 Astronomical Institute Anton Pannekoek, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
3 Institute for Advanced Study, Princeton, NJ 08540, USA

Received 24 June 1996 / Accepted 19 December 1996


Star clusters with a high central density contain an ecological network of evolving binaries, affected by interactions with passing stars, while in turn affecting the energy budget of the cluster as a whole by giving off binding energy. This is the first paper in a series aimed at providing the tools for increasingly realistic simulations of these ecological networks.

Here we model the core of a globular star cluster. The two main approximations are: a density of stars constant in space and time, and a purely single star population in which collisions between the evolving stars are modeled. In future papers in this series, we will relax these crude approximations. Here, however, they serve to set the stage before proceeding to the additional complexity of binary star interactions, in paper II, and background dynamical evolution, in later papers.

Key words: methods: numeric - celestial mechanics: stellar dynamics - stars: evolution - stars: blue stragglers - globular clusters: general

Send offprint requests to: Simon Portegies Zwart

© European Southern Observatory (ESO) 1997

Online publication: October 30, 1997
Last change: March 24, 1998