301 citations · 6.3k across the 162 of their papers we have counts for
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Magnetic braking during direct collapse black hole formation
Muhammad A. Latif, Dominik R. G. Schleicher
Magnetic fields are expected to be efficiently amplified during the formation of the first massive black holes via the small-scale dynamo and in the presence of strong accretion sh…
Survival of fossil fields during the pre-main sequence evolution of intermediate-mass stars
Dominik R. G. Schleicher, Juan Pablo Hidalgo, Daniele Galli
Chemically peculiar Ap and Bp stars host strong large-scale magnetic fields in the range of ~G up to ~kG, which are often considered to be the origin of fossil magnetic fi…
Effects of the centrifugal force in stellar dynamo simulations
Felipe H. Navarrete, Petri J. Käpylä, Dominik R. G. Schleicher +1
The centrifugal force is often omitted from simulations of stellar convection either for numerical reasons or because it is assumed to be weak compared to the gravitational force.…
Origin of magnetism in early-type stars
J. P. Hidalgo, P. J. Käpylä, C. A. Ortiz-Rodríguez +3
According to our understanding of stellar evolution, early-type stars have radiative envelopes and convective cores due to a steep temperature gradient produced by the CNO cycle. S…
Formation of supermassive stars in the first star clusters
Bastián Reinoso, Ralf S. Klessen, Dominik Schleicher +2
The formation of supermassive stars is believed to be an essential intermediate step for the formation of the massive black hole seeds that become the supermassive black holes powe…
The physical origin of super-competitive accretion during the formation of the first supermassive black holes
Dominik R. G. Schleicher, Bastián Reinoso, Ralf S. Klessen
Numerical simulations have shown the occurence of a scenario termed ''super-competitive accretion'', a term that describes a situation where only the central few objects grow super…