  Various galactic globular clusters display abundance anomalies that affect
the morphology of their colour-magnitude diagrams. In this paper we consider
the possibility of helium enhancement in the anomalous horizontal branch of NGC
2808. We examine the dynamics of a self-enrichment scenario in which an initial
generation of stars with a top-heavy initial mass function enriches the
interstellar medium with helium via the low-velocity ejecta of its asymptotic
giant branch stars. This enriched medium then produces a second generation of
stars which are themselves helium-enriched. We use a direct N-body approach to
perform five simulations and conclude that such two-generation clusters are
both possible and would not differ significantly from their single-generation
counterparts on the basis of dynamics. We find, however, that the stellar
populations of such clusters would differ from single-generation clusters with
a standard initial mass function and in particular would be enhanced in white
dwarf stars. We conclude, at least from the standpoint of dynamics, that
two-generation globular clusters are feasible.
