activity
20222026
most citedFormation of supermassive stars in the first star clusters

43 citations · 94 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Quantifying collision-driven mass loss in supermassive star formation: the role of stellar structure and accretion

P. A. Solar, B. Reinoso, D. R. G. Schleicher +1

Observations of high-redshift galaxies with JWST have renewed interest in scenarios where supermassive stars form via runaway stellar collisions in dense clusters, yet the impact o…

astro-ph.GA2026

Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes

Dominik R. G. Schleicher, Matías Liempi, Mirek Giersz +11

The James Webb Space Telescope (JWST) has detected, through gravitational lensing, several young massive star clusters (YMCs), which are considered as relevant building blocks of h…

astro-ph.GA2025★ 7 cited

Formation of supermassive stars in the first stellar clusters: Dependence on the gas temperature

P. A. Solar, B. Reinoso, D. R. G. Schleicher +2

The origin of supermassive black holes is an open question that has been explored considering gas- and collision-based formation channels to explain the high number of quasars obse…

astro-ph.GA2024★ 3 cited

Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object

Jorge Saavedra-Bastidas, Dominik R. G. Schleicher, Ralf S. Klessen +7

The formation of massive objects via gravitational collapse is relevant both for explaining the origin of the first supermassive black holes and in the context of massive star form…

astro-ph.GA2023★ 43 cited

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…

astro-ph.GA2022★ 41 cited

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…