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- W3102024863 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 105 to 107 M⊙, 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 108–9 M⊙ can form at the same time, and appear to be part of a different class of objects, being more extended and rotating." @default.
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- W3102024863 date "2008-09-01" @default.
- W3102024863 modified "2023-10-18" @default.
- W3102024863 title "High-resolution simulations of galaxy mergers: resolving globular cluster formation" @default.
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- W3102024863 doi "https://doi.org/10.1111/j.1745-3933.2008.00511.x" @default.
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