356 citations · 4k across the 80 of their papers we have counts for
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Formation of massive black holes via collisions and accretion
D. R. G. Schleicher, M. A. Fellhauer, T. Boekholt +13
To explain the observed population of supermassive black holes at z~7, very massive seed black holes or, alternatively, super-Eddington scenarios are needed to reach final masses o…
Gas expulsion in highly substructured embedded star clusters
J. P. Farias, M. Fellhauer, R. Smith +2
We investigate the response of initially substructured, young, embedded star clusters to instantaneous gas expulsion of their natal gas. We introduce primordial substructure to the…
Collisions in Primordial Star Clusters: Formation Pathway for intermediate mass black holes
B. Reinoso, D. R. G. Schleicher, M. Fellhauer +2
Collisions were suggested to potentially play a role in the formation of massive stars in present day clusters, and have likely been relevant during the formation of massive stars…
Formation of massive seed black holes via collisions and accretion
T. C. N. Boekholt, D. R. G. Schleicher, M. Fellhauer +4
Models aiming to explain the formation of massive black hole seeds, and in particular the direct collapse scenario, face substantial difficulties. These are rooted in rather ad hoc…