Star cluster at a distance of 16pc from the Galactic center
Simulation of a star cluster with 12288 stars (taken from a Scalo mass function between 0.3 and 100 solar mass) at a distance of 16pc from the Galactic center. At this instant the cluster has an age of about 1.0 million years. The cluster has a diameter (virial radius) of 0.25pc. The colors and sizes of the stars represent their spectral type and apparent luminosity. The background object represents the Galactic center with part of a spiral dust arm. The image is comparable to the Arches cluster model, which has similar initial conditions but slightly closer to the Galactic center.
As in the Arches cluster model, many stars are currently leaving the cluster. We are looking from the stream of stars which leave the cluster through the thrird Lagrangian point in the combined potential of the Galaxy and cluster. These stars have a circumgalactic velocities slightly higher than the bulk motion of the cluster.
All calculations are performed on the GRAPE-6 at Tokyo University using the starlab toolset. The trajectories of the stars are calculated with kira and the evolution of the stars was computed with SeBa (for details see Portegies Zwart, Makino, McMillan and Hut 2002, ApJ in press or the more theoretical paper by Portegies Zwart and McMillan ApJ submitted).
The simulation can best be compared with the observed Quintuplet star cluster. This cluster contains about 20000 stars and is located at a (projected) distance of 35pc from the Galactic center. Even with the Hubble Space Telescope only the brightest stars are visible in this image. In this hubble image, however, it is attempted to represent the stars with their true colors, as is done in the simulated image.