Figure: Effective potential isolines and comparison with a simulation. From: A. Ernst, A. Just, P. Berczik, M. Petrov, Calibration of radii and masses of open clusters with a simulation, 2010, A&A, 524, A62 |
Figure: Dissolving cluster in the Galactic centre. From: A. Ernst, A. Just, R. Spurzem, On the dissolution of star clusters in the Galactic centre. I. Circular orbits, 2009, MNRAS 399, 141 |
Movie: A star cluster spiralling into the Galactic Center on a circular orbit, N = 5000, M_cl = 10^6 M_sol, V0 = V_cir, King W0 = 9 |
Movie: A star cluster spiralling into the Galactic Center on a rosette orbit, N = 5000, M_cl = 10^6 M_sol, V0 = 0.5 V_cir, King W0 = 9 |
Movie: A star cluster spiralling into the Galactic Center on an eccentric rosette orbit, N = 5000, M_cl = 10^6 M_sol, V0 = 0.25 V_cir, King W0 = 9 |
Movie: A dissolving star cluster. Made with POVRAY. |