output
20052026
most citedGravitational Wave Astronomy With TianQin

56 citations

22 papers

astro-ph.HE2026

Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots

Ataru Tanikawa, Masaru Shibata, Kunihito Ioka

Using gravitational -body simulations, we investigate the evolution of mass and spin for very massive stars (VMSs) in dense star clusters, which could subsequently evolve into L…

astro-ph.GA2026

Investigating the formation channel of GW231123: Population III stars or hierarchical mergers?

Federico Angeloni, Konstantinos Kritos, Raffaella Schneider +5

The gravitational wave event GW231123, with component black hole masses lying within or above the pair-instability mass gap, poses a significant challenge to current stellar evolut…

astro-ph.GA2026

Direct N-body simulations of rotating and extremely massive Population III star clusters

Kai Wu, Ataru Tanikawa, Francesco Flammini Dotti +6

Aims. We present eight direct N-body simulations with NBODY6++GPU of extremely massive, initially rotating Population III star clusters with 1.01 x 10^5 stars. Methods. Our models…

astro-ph.SR2026★ 1 cited

Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects

Ataru Tanikawa, Akito Tajitsu, Satoshi Honda +5

We have discovered a compact hierarchical triple main-sequence star system, which is cataloged as Gaia DR3 1010268155897156864 or TIC 21502513. Hereafter, we call it ``G1010''. G10…

astro-ph.EP2025★ 2 cited

Cosmic-Ray Bath in a Past Supernova Gives Birth to Earth-Like Planets

Ryo Sawada, Hiroyuki Kurokawa, Yudai Suwa +3

A key question in astronomy is how ubiquitous Earth-like rocky planets are. The formation of terrestrial planets in our solar system was strongly influenced by the radioactive deca…

astro-ph.SR2025★ 1 cited

Two unseen massive white dwarf candidates in close binaries

Yuta Shiraishi, Kenta Hotokezaka, Kento Masuda +10

We report the discovery of two binary systems, each consisting of a slightly bloated G-type main-sequence star and an unseen companion, identified through photometric data from TES…