356 citations · 4k across the 80 of their papers we have counts for
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Formation of SMBH seeds in Pop III star clusters through collisions : the importance of mass loss
P. J. Alister Seguel, D. R. G. Schleicher, T. C. N. Boekholt +2
Runaway collisions in dense clusters may lead to the formation of supermassive black hole (SMBH) seeds, and this process can be further enhanced by accretion, as recent models of S…
Modelling the Canes Venatici I dwarf spheroidal galaxy
D. R. Matus Carillo, M. Fellhauer, A. G. Alarcon Jara +2
The aim of this work is to find a progenitor for Canes Venatici I (CVn I), under the assumption that it is a dark matter free object that is undergoing tidal disruption. With a sim…
Stirring up an embedded star cluster with a moving gas filament
D. Matus Carrillo, M. Fellhauer, A. Stutz
We perform simulations to test the effects of a moving gas filament on a young star cluster (i.e. the "Slingshot" Model). We model Orion Nebula Cluster-like clusters as Plummer sph…
The formation of compact dwarf ellipticals through merging star clusters
F. Urrutia Zapata, M. Fellhauer, A. G. Alarcon Jara +2
In the last decades, extended old stellar clusters have been observed. These extended objects cover a large range in masses, from extended clusters or faint fuzzies to ultra compac…