Star cluster ecology — IV. Dissection of an open star cluster: photometry
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 calcu...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2001-02, Vol.321 (2), p.199-226 |
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