most citedUnveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation

1 citations · 3 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

An Explicit M1 Radiation-hydrodynamics Scheme for 3D Protostellar Evolution

Kazutaka Kimura, Kazuyuki Sugimura, Takashi Hosokawa +2

We present a radiation-hydrodynamics (RHD) scheme that enables 3D simulations resolving both protostellar interiors and their surrounding accretion flows within a single framework,…

astro-ph.GA2025★ 1 cited

Neural-Network Chemical Emulator for First-Star Formation: Robust Iterative Predictions over a Wide Density Range

Sojun Ono, Kazuyuki Sugimura

We present a neural-network emulator for the thermal and chemical evolution in Population III star formation. The emulator accurately reproduces the thermochemical evolution over a…

astro-ph.GA2025★ 1 cited

Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation

Yurina Nakazato, Kazuyuki Sugimura, Akio K. Inoue +1

Recent multi-wavelength observations by JWST and ALMA are unveiling both ionized and neutral ISM components in high-redshift () galaxies. In this work, we investigate the orig…

astro-ph.GA2024★ 1 cited

Impact of Turbulent Magnetic Fields on Disk Formation and Fragmentation in First Star Formation

Kenji Eric Sadanari, Kazuyuki Omukai, Kazuyuki Sugimura +2

Recent cosmological hydrodynamic simulations have suggested that the first stars in the universe often form as binary or multiple systems. However, previous studies typically overl…

astro-ph.GA2024

Gas Dynamical Friction on Accreting Objects

Tomoya Suzuguchi, Kazuyuki Sugimura, Takashi Hosokawa +1

The drag force experienced by astronomical objects moving through gaseous media (gas dynamical friction) plays a crucial role in their orbital evolution. Ostriker (1999) derived a…