41 citations · 70 across the 3 of their papers we have counts for
5 papers
Origin of supermassive black holes in massive metal-poor protoclusters
D. R. G. Schleicher, B. Reinoso, M. Latif +6
While large numbers of supermassive black holes have been detected at z>6, their origin is still essentially unclear. Numerical simulations have shown that the conditions for the c…
Stellar collisions in flattened and rotating Pop. III star clusters
M. Z. C. Vergara, D. R. G. Schleicher, T. C. N. Boekholt +4
Fragmentation often occurs in disk-like structures, both in the early Universe and in the context of present-day star formation. Supermassive black holes (SMBHs) are astrophysical…
Small-N Collisional Dynamics V: Beyond the Realm of Not-So-Small-N
Carlos Barrera, Nathan W. C. Leigh, Bastián Reinoso +2
Direct collisions between finite-sized particles occur commonly in many areas of astrophysics. Such collisions are typically mediated by chaotic, bound gravitational interactions i…
The effects of a background potential in star cluster evolution: a delay in the relaxation time-scale and runaway collision processes
B. Reinoso, D. R. G. Schleicher, M. Fellhauer +2
Runaway stellar collisions in dense star clusters are invoked to explain the presence of very massive stars or blue stragglers in the center of those systems. This process has also…
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…