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Evolution of star cluster systems in isolated galaxies: first results from directN-body simulations
2016
Monthly notices of the Royal Astronomical Society
The evolution of star clusters is largely affected by the tidal field generated by the host galaxy. It is thus in principle expected that under the assumption of an "universal" initial cluster mass function the properties of the evolved present-day mass function of star cluster systems should show a dependency on the properties of the galactic environment in which they evolve. To explore this expectation a sophisticated model of the tidal field is required in order to study the evolution of
doi:10.1093/mnras/stw1827
fatcat:tdkrsb55krgrxl5njil6yf3oyy