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20222026
most citedRapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters

16 citations · 43 across the 10 of their papers we have counts for

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astro-ph.HE2023

The Dragon-II simulations -- III. Compact binary mergers in clusters with up to 1 million stars: mass, spin, eccentricity, merger rate and pair instability supernovae rate

Manuel Arca Sedda, Albrecht W. H. Kamlah, Rainer Spurzem +4

Compact binary mergers forming in star clusters may exhibit distinctive features that can be used to identify them among observed gravitational-wave (GW) sources. Such features lik…