paper

High-resolution simulations of galaxy mergers: Resolving globular cluster formation

arXiv:0806.1386 · doi:10.1111/j.1745-3933.2008.00511.x

Abstract

Massive star clusters observed in galaxy mergers are often suggested to be progenitors of globular clusters. To study this hypothesis, we performed the highest resolution simulation of a gas-rich galaxy merger so far. The formation of massive star clusters of 10^5 to 10^7 Mo, triggered by the galaxy interaction, is directly resolved in this model. We show that these clusters are tightly bound structures with little net rotation, due to evolve into compact long-lived stellar systems. Massive clusters formed in galaxy mergers are thus robust candidates for progenitors of long-lived globular clusters. The simulated cluster mass spectrum is consistent with theory and observations. Tidal dwarf galaxies of 10^8-9 Mo can form at the same time, and appear to be part of a different class of objects, being more extended and rotating.

MNRAS letters accepted. Version with high-resolution figures available at http://aramis.obspm.fr/~bournaud/GC.pdf

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