Kazuyuki Sugimura

Physics and Astronomy · Physical Sciences

22h-index1.5kcitations111works4.52yr avg
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Research Topics

Astrophysics and Star Formation Studies(24), Turbomachinery Performance and Optimization(21), Stellar, planetary, and galactic studies(18), Astrophysical Phenomena and Observations(17), Galaxies: Formation, Evolution, Phenomena(13)

Publications111 total

Unveiling the Ionized and Neutral ISM at <i>z</i> &gt; 10: The Origin of [O <scp>iii</scp> ] /[C <scp>ii</scp> ] Ratios from a Subparsec Resolution Radiative Transfer Simulation
The Astrophysical Journal·2026Open Access
Neural-network Chemical Emulator for First-star Formation: Robust Iterative Predictions Over a Wide Density Range
The Astrophysical Journal·2025Open Access
Seeding Cores: A Pathway for Nuclear Star Clusters from Bound Star Clusters in the First Billion Years
The Open Journal of Astrophysics·2025· 3 citedOpen Access
Unveiling the Ionized and Neutral ISM at z &gt; 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation
arXiv (Cornell University)·2025Open Access
Seeding Cores: A Pathway for Nuclear Star Clusters from Bound Star Clusters in the First Billion Years
arXiv (Cornell University)·2025Open Access
Violent Starbursts and Quiescence Induced by Far-ultraviolet Radiation Feedback in Metal-poor Galaxies at High Redshift
The Astrophysical Journal·2024· 18 citedOpen Access
Impact of turbulent magnetic fields on disk formation and fragmentation in first star formation
Publications of the Astronomical Society of Japan·2024· 11 citedOpen Access
Impact of Turbulent Magnetic Fields on Disk Formation and Fragmentation in First Star Formation
arXiv (Cornell University)·2024· 1 citedOpen Access
Gas Dynamical Friction on Accreting Objects
The Astrophysical Journal·2024· 9 citedOpen Access
On the origin of outward migration of Population III stars
Monthly Notices of the Royal Astronomical Society·2024· 7 citedOpen Access
Gas Dynamical Friction on Accreting Objects
arXiv (Cornell University)·2024Open Access
Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamic Simulations
The Astrophysical Journal·2023· 25 citedOpen Access
On the origin of outward migration of Population III stars
arXiv (Cornell University)·2023Open Access
Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamics Simulations
arXiv (Cornell University)·2023· 2 citedOpen Access
3D Radiation-hydrodynamic Simulations Resolving Interior of Rapidly Accreting Primordial Protostar
The Astrophysical Journal·2023· 17 citedOpen Access
Star cluster formation and survival in the first galaxies
Monthly Notices of the Royal Astronomical Society·2023· 23 citedOpen Access
Population III star formation in an X-ray background: III. Periodic radiative feedback and luminosity induced by elliptical orbits
Monthly Notices of the Royal Astronomical Society·2023· 20 citedOpen Access
3D Radiation-Hydrodynamic Simulations Resolving Interior of Rapidly Accreting Primordial Protostar
arXiv (Cornell University)·2023Open Access
Star Cluster Formation and Survival in the First Galaxies
arXiv (Cornell University)·2022Open Access
Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion
Monthly Notices of the Royal Astronomical Society·2022· 15 citedOpen Access
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Frequent Co-authors

Kazuyuki Omukai(12), Takashi Hosokawa(9), Tomoaki Matsumoto(7), Shigeru Obayashi(7), Shinkyu Jeong(7), Massimo Ricotti(6), Hidenobu Yajima(5), Jongwon Park(5), Ichiro Azuma(4), Hiromi Kobayashi(4), Hideo Nishida(4), Kenji Eric Sadanari(3), Kengo Tomida(3), Takeshi Kimura(3), I Saiki(2), J Murata(2), Norio Nishi(2), Hiroaki Shimokawa(2), Hajime Fukushima(2), Daisuke Toyouchi(2)