155 citations · 894 across the 30 of their papers we have counts for
30 papers
Seeding Cores: A Pathway for Nuclear Star Clusters from Bound Star Clusters in the First Billion Years
Fred Angelo Batan Garcia, Massimo Ricotti, Kazuyuki Sugimura
We model the formation of star clusters in a dwarf galaxy progenitor during the first of cosmic history using a cosmological radiation-hydrodynamic simulation with…
Violent starbursts and quiescence induced by FUV radiation feedback in metal-poor galaxies at high-redshift
Kazuyuki Sugimura, Massimo Ricotti, Jongwon Park +2
JWST observations of galaxies at suggest that they are more luminous and clumpier than predicted by most models, prompting several proposals on the physics of star for…
Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamics Simulations
Kazuyuki Sugimura, Tomoaki Matsumoto, Takashi Hosokawa +2
We study the formation of Pop III stars by performing radiation hydrodynamics simulations for three different initial clouds extracted from cosmological hydrodynamics simulations.…
On the origin of outward migration of Population III stars
Jongwon Park, Massimo Ricotti, Kazuyuki Sugimura
Outward migration of massive binary stars or black holes in their circumbinary disc is often observed in simulations and it is key to the formation of wide black hole binaries. Usi…
3D Radiation-Hydrodynamic Simulations Resolving Interior of Rapidly Accreting Primordial Protostar
Kazutaka Kimura, Takashi Hosokawa, Kazuyuki Sugimura +1
Direct collapse of supermassive stars is a possible pathway to form supermassive black hole seeds at high redshifts. Whereas previous three-dimensional (3D) simulations demonstrate…
Star Cluster Formation and Survival in the First Galaxies
Fred Angelo Batan Garcia, Massimo Ricotti, Kazuyuki Sugimura +1
Using radiation-hydrodynamic cosmological simulations, we present a detailed ( pc resolution), physically motivated portrait of a typical-mass dwarf galaxy before the epoch of…