The dynamics of self-gravitating globular cluster-like systems, containing N = 10(5) stars, has been simulated for 6 - 10 crossing times. We followed the evolution of three different spherical systems. The first two are quasi-virialized clusters, (with and without the presence, in the centre of mass, of a black hole); the third case regards the initial violent collapse of a spherical system.
The dynamics of self-gravitating globular cluster-like systems, containing N = 10(5) stars, has been simulated for 6 - 10 crossing times. We followed the evolution of three different spherical systems. The first two are quasi-virialized clusters, (with and without the presence, in the centre of mass, of a black hole); the third case regards the initial violent collapse of a spherical system.
N-body simulations of Globular Cluster-like systems / P., DI MATTEO; P., Miocchi; CAPUZZO DOLCETTA, Roberto Angelo. - STAMPA. - 296:(2003), pp. 572-573. (Intervento presentato al convegno New Horizons in Globular Cluster Astronomy, Padova tenutosi a Padova nel 24-28 giugno 2002).
N-body simulations of Globular Cluster-like systems
CAPUZZO DOLCETTA, Roberto Angelo
2003
Abstract
The dynamics of self-gravitating globular cluster-like systems, containing N = 10(5) stars, has been simulated for 6 - 10 crossing times. We followed the evolution of three different spherical systems. The first two are quasi-virialized clusters, (with and without the presence, in the centre of mass, of a black hole); the third case regards the initial violent collapse of a spherical system.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
