Star cluster ecology -- IV. Dissection of an open star cluster: photometry

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

Type: Article

Publication Date: 2001-02-21

Citations: 335

DOI: https://doi.org/10.1046/j.1365-8711.2001.03976.x

Abstract

The evolution of star clusters is studied using N-body simulations in which the evolution of single stars and binaries is taken self-consistently into account. Initial conditions are chosen to represent relatively young Galactic open clusters, such as the Pleiades, Praesepe and the Hyades. The calculations include a realistic mass function, primordial binaries and the external potential of the parent Galaxy.

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Monthly Notices of the Royal Astronomical Society - View - PDF
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