most citedGW231123 Formation from Population III Stars: Isolated Binary Evolution

4 citations · 7 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.SR20264 cited

GW231123 Formation from Population III Stars: Isolated Binary Evolution

Ataru Tanikawa, Shuai Liu, WeiWei Wu +2

GW231123 is a merger of two black holes (BHs) with estimated masses exceeding , making them the most massive BHs discovered to date via gravitational wave (GW…

astro-ph.GA20263 cited

Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales

Takumi S. Tanaka, John D. Silverman, Kazuhiro Shimasaku +56

``Little Red Dots'' (LRDs) are an abundant high-redshift population newly discovered by the James Webb Space Telescope (JWST) and considered to be an early growth phase of supermas…

astro-ph.GA2026

Tree-ring structure of Galactic bar resonance in N-body simulations

Rimpei Chiba, Michiko Fujii, Junichi Baba +2

We study the structure and evolution of the galactic bar's resonant phase-space in self-consistent N-body simulations of the Milky Way, with and without perturbations from the Sagi…

astro-ph.GA2026

SIRIUS: The relation between the diversity of dwarf galaxies and their formation histories

Chi-Hong Lin, Michiko S Fujii, Takayuki R Saitoh +1

Low-mass dwarf galaxies () are fundamental cosmological building blocks, yet the physical processes driving their structural diversity remain…

astro-ph.GA2025

On the Formation of GW231123 in Population III Star Clusters

Shuai Liu, Long Wang, Ataru Tanikawa +2

GW231123 is a binary black hole merger whose primary component lies within or above the pair-instability mass gap, while the secondary component falls within this gap. The standard…

astro-ph.SR2025

Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs

Savannah Cary, Michiko Fujii, Long Wang +1

Studying compact-object binary mergers in star clusters is crucial for understanding stellar evolution and dynamical interactions in galaxies. Open clusters in particular are more…