Ataru Tanikawa

Tokyo University of the Arts — Japan

Physics and Astronomy · Physical Sciences

25h-index1.6kcitations115works5.42yr avg
OpenAlex↗ORCID↗Google Scholar↗Lab page↗

Accepting Students?

No reports yet. Know if this professor is taking students?

Research Topics

Pulsars and Gravitational Waves Research(50), Gamma-ray bursts and supernovae(47), Stellar, planetary, and galactic studies(43), Astrophysical Phenomena and Observations(31), Astronomy and Astrophysical Research(21)

Publications115 total

Two unseen massive white dwarf candidates in close binaries
Publications of the Astronomical Society of Japan·2025Open Access
Cosmic-ray bath in a past supernova gives birth to Earth-like planets
Science Advances·2025Open Access
Rapid formation of a very massive star (&gt;50000 M <sub>⊙</sub> ), and subsequently, of an IMBH, from runaway collisions
Astronomy and Astrophysics·2025· 2 citedOpen Access
On the Formation of GW231123 in Population III Star Clusters
The Astrophysical Journal Letters·2025· 3 citedOpen Access
On the Formation of GW231123 in Population III Star Clusters
arXiv (Cornell University)·2025Open Access
Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs
The Astrophysical Journal·2025· 1 citedOpen Access
GW231123 Formation from Population III Stars: Isolated Binary Evolution
arXiv (Cornell University)·2025Open Access
Compact Binary Formation in Open Star Clusters III: Probability of Binary Black Holes Hidden Inside of Gaia Black Hole Binary
The Open Journal of Astrophysics·2025· 2 citedOpen Access
Pair-instability Gap Black Holes in Population III Star Clusters: Pathways, Dynamics, and Gravitational-wave Implications
The Astrophysical Journal·2025· 3 citedOpen Access
Unevolved Li-rich stars at low metallicity: A possible formation pathway through novae
Astronomy and Astrophysics·2025· 1 citedOpen Access
The hydrodynamics of double white dwarf mergers
Elsevier eBooks·2025
Rapid formation of a very massive star &gt;50000 $M_\odot$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
arXiv (Cornell University)·2025Open Access
Pair-Instability Gap Black Holes in Population III Star Clusters: Pathways, Dynamics, and Gravitational Wave Implications
arXiv (Cornell University)·2025Open Access
Gravitational wave astronomy with TianQin
Reports on Progress in Physics·2025· 28 cited
Gravitational collapse of white dwarfs to neutron stars: From initial conditions to explosions with neutrino-radiation hydrodynamics simulations
Publications of the Astronomical Society of Japan·2024· 3 cited
Double white dwarf mergers and type Ia supernovae
2024Open Access
Gravitational Wave Astronomy With TianQin
arXiv (Cornell University)·2024· 3 citedOpen Access
Merging hierarchical triple black hole systems with intermediate-mass black holes in population III star clusters
Monthly Notices of the Royal Astronomical Society·2024· 16 citedOpen Access
Compact Binary Formation in Open Star Clusters III: Probability of Binary Black Holes Hidden in Gaia Black Hole Binary
arXiv (Cornell University)·2024· 1 citedOpen Access
Simulations predict intermediate-mass black hole formation in globular clusters
Science·2024· 31 citedOpen Access
page 1 of 6Next →

Frequent Co-authors

Michiko S. Fujii(13), Tomoya Kinugawa(8), Long Wang(8), M. Shikauchi(6), Nozomu Tominaga(6), Takashi Yoshida(5), Alessandro A. Trani(5), Jun Kumamoto(5), Keigo Nitadori(4), Norita Kawanaka(4), Junichiro Makino(4), Fumihiko Usui(4), Ko Arimatsu(4), Seitaro Urakawa(4), Shigeyuki Sako(4), Tomoki Morokuma(4), Masaomi Tanaka(4), Hajime Susa(3), Hideyuki Umeda(3), Naohito Nakasato(3)