Monte Carlo modelling of globular star clusters: Intermediate Mass Black Holes formation and their observational properties
Le 30 septembre 2016 De 10h30 à 12h00 Mirek GIERSZ Nicolaus Copernicus Astronomical Center, Varsovie I will very briefly talk about the basic assumptions behind the Monte Carlo method and discuss why this method is so fast and flexible for large star cluster simulations. I...


