Star cluster ecology – V. Dissection of an open star cluster: spectroscopy

Simon Portegies Zwart, Piet Hut, Stephen L. W. McMillan, Junichiro Makino

Type: Article

Publication Date: 2004-06-11

Citations: 19

DOI: https://doi.org/10.1111/j.1365-2966.2004.07709.x

Abstract

We have modelled in detail the evolution of rich open star clusters such as NGC 2516, NGC 2287, Pleiades, Praesepe, Hyades, NGC 2660 and 3680, using simulations that include stellar dynamics as well as the effects of stellar evolution. The dynamics is modelled via direct N-body integration, while the evolution of single stars and binaries is followed through the use of fitting formulae and recipes. The feedback of stellar and binary evolution on the dynamical evolution of the stellar system is taken into account self-consistently.

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