248 citations · 2.3k across the 78 of their papers we have counts for
7 papers · 1 filter
Black hole formation in the context of dissipative dark matter
M. A. Latif, A. Lupi, D. R. G. Schleicher +3
Black holes with masses of dwell in the centers of most galaxies, but their formation mechanisms are not well known. A subdominant dissipative component o…
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…
Impact of radiation backgrounds on the formation of massive black holes
V. B. Díaz, D. R. G. Schleicher, S. Bovino +4
The presence of supermassive black holes (SMBHs) of a few billion solar masses at very high redshift has motivated us to study how these massive objects formed during the first bil…
Synthetic observations of HD towards high-mass starless cores
Joaquin. Zamponi F., Dominik R. G. Schleicher, Stefano Bovino +3
Young massive stars are usually found embedded in dense and massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteratio…
Star formation at high redshift
P. Fibla, S. Bovino, R. Riaz +4
We present here a three-dimesional hydrodynamical simulation for star formation. Our aim is to explore the effect of the metal-line cooling on the thermodynamics of the star-format…
Thermodynamics and Chemistry of the Early Universe
Stefano Bovino, Daniele Galli
The interplay between chemistry and thermodynamics determines the final outcome of the process of gravitational collapse and sets the conditions for the formation of the first cosm…
The formation of protostellar binaries in primordial minihalos
Rafeel Riaz, Stefano Bovino, Siegfried Vanaverbeke +1
The first stars are known to form in primordial gas, either in minihalos with about ~M or so-called atomic cooling halos of about ~M. Simulations have s…