PI: Miklos Peuten
Co-I: Mark Gieles
Other active participants: Alice Zocchi, Antonio Sollima, Vincent Henault-Brunet, Anna Lisa Varri

Questions to address:

1. Can the mass segregation be reproduced by multi-mass King models?
2. How important is the effect of mass segregation?
3. How correct is the assumption of energy equipartition?

Data: Snapshots of simulations with a mass function (no stellar evolution) to be uploaded shortly.

The relevant snapshots from simulations with a mass function are available in section B of the Mock data page.

The definition of the stellar types (KSTAR) used in the NBODY6 snapshots can be found in the Appendix section of the Mock data page.

Anisotropy profile of different components in multi-mass clusters. Left: N-body simulation. Right: Three-component multi-mass Michie model.