The Promiscuous Nature of Stars in Clusters
arXiv:astro-ph/0201217 · doi:10.1086/339495
Abstract
The recent availability of special purpose computers designed for calculating gravitational interactions of N-bodies at extremely high speed has provided the means to model globular clusters on a star-by-star basis for the first time. By endeavouring to make the N-body codes that operate on these machines as realistic as possible, the addition of stellar evolution being one example, much is being learnt about the interaction between the star cluster itself and the stars it contains. A fascinating aspect of this research is the ability to follow the orbits of individual stars in detail and to document the formation of observed exotic systems. This has revealed that many stars within a star cluster lead wildly promiscuous lives, interacting, often intimately and in rapid succession, with a variety of neighbours.
15 pages, 1 figure, to appear in the Astrophysical Journal
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- Gravitational Radiation from Intermediate-Mass Black Holes
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- Survey for Transiting Extrasolar Planets in Stellar Systems: I. Fundamental Parameters of the Open Cluster NGC 1245
- Modelling Collision Products of Triple-Star Mergers
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- A Blue Straggler Binary System with at least Three Progenitors in the Core of a Globular Cluster?
- Erupting Dwarf Novae in the Large Magellanic Cloud