activity
20242026
most citedNitrogen enhancement of GN-z11 by metal pollution from supermassive stars

1 citations · 1 across the 2 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

SIRIUS Project: Dynamical Evolution of Primordial Binaries during Star Cluster Formation

Naoto Harada, Michiko S. Fujii, Takayuki R. Saitoh +1

Binary populations are closely linked to the star formation process; however, their primordial properties can be changed by subsequent dynamical interactions within their natal clu…

astro-ph.GA20261 cited

Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars

Sho Ebihara, Michiko S. Fujii, Takayuki R. Saitoh +4

Spectroscopic observations by the James Webb Space Telescope (JWST) have revealed young, compact, high-redshift () galaxies with high nitrogen-to-oxygen (N/O) ratios. GN-z11 at…

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.GA2026

SIRIUS: Dark matter cusp evolution in dense dwarf galaxies

Katsuhiro Kaneko, Takayuki R. Saitoh, Yutaka Hirai +1

Dwarf galaxies have a wide variety of structures, such as dark matter (DM) distribution, stellar-to-halo mass ratio, and stellar density. Recent high-resolution simulations have sh…

astro-ph.GA2025

Bursty star formation, chemical enrichment, and star cluster formation in numerical analogues of GN-z11

Takayuki R. Saitoh, Yutaka Hirai, Michiko S. Fujii +1

The James Webb Space Telescope reveals anomalous nitrogen enrichment (high N/O ratios) in compact, star-forming galaxies, such as GN-z11 at . The origin of this chemical s…

astro-ph.SR2025

A New Subclass of Carbon-Enhanced Metal-Poor Stars at Extremely Low Metallicity

Young Sun Lee, Timothy C. Beers, Yutaka Hirai +4

We report the discovery of a new subclass of carbon-enhanced metal-poor (CEMP) stars, characterized by high absolute carbon abundances (A(C) > 7.39) and extremely low metallicity (…