activity
19982026
most citedLow-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution

274 citations · 321 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

High-Precision Near-Infrared Abundances of Solar Analogs in the YJ Bands

Noriyuki Matsunaga, Takuji Tsujimoto, Daisuke Taniguchi +12

We present a near-infrared abundance analysis of 46 solar analogs with known ages, observed with the WINERED WIDE-mode spectrograph at a resolution of . Using an empi…

astro-ph.GA2026★ 1 cited

Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration

Takuji Tsujimoto, Daisuke Taniguchi, Alejandra Recio-Blanco +2

Solar twins are among the most powerful tracers of Galactic disk evolution owing to their unique property of sharing nearly solar metallicities ([Fe/H] ~ 0) while spanning a wide r…

astro-ph.GA2026★ 3 cited

On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid

G. Bono, V. F. Braga, M. Fabrizio +54

We introduce a new photometric catalog of RR Lyrae variables (RRLs, 300,000) mainly based on data available in public datasets. We also present the largest and most homogeneo…

astro-ph.SR2026★ 2 cited

Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages

Daisuke Taniguchi, Patrick de Laverny, Alejandra Recio-Blanco +2

[Abbreviated] Context. Solar twins, stars whose stellar parameters (Teff, log g, and [M/H]) are very close to the Solar ones, offer a unique opportunity to investigate Galactic arc…

astro-ph.GA2025

The VISCACHA survey XIV. Chemical evolution history of the SMC: The Southern Bridge Clusters

Sasi Saroon, B. Dias, T. Tsujimotto +18

The chemical evolution history of the Small Magellanic Cloud (SMC) is complex and is best understood through a comprehensive analysis of star clusters across its various regions. T…

astro-ph.GA2025

An Ultra-Faint, Chemically Primitive Galaxy Forming in the Reionization Era

Kimihiko Nakajima, Masami Ouchi, Yuichi Harikane +9

The formation of the first stars and galaxies marked the onset of chemical enrichment, yet direct observations of such primordial systems remain elusive. Here we present James Webb…

astro-ph.GA2025

Discovery of WINERED-HVS1: A metal-rich hyper-velocity star candidate ejected from the Galactic center

Kohei Hattori, Daisuke Taniguchi, Takuji Tsujimoto +4

We report the discovery of a metal-rich red giant star, WINERED-HVS1, which is a candidate for a hyper-velocity star (HVS). Its past trajectory suggests that this star may have bee…

astro-ph.GA2025★ 8 cited

MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars

Daisuke Taniguchi, Noriyuki Matsunaga, Naoto Kobayashi +11

[Abbreviated] Context. Given their high luminosities (L>~10^4Lsun), red supergiants (RSGs) are good tracers of the chemical abundances of the young stellar population in the Milky…

astro-ph.GA2024★ 11 cited

Solar System Migration Points to a Renewed Concept: Galactic Habitable Orbits

Junichi Baba, Takuji Tsujimoto, Takayuki R. Saitoh

Astrophysical evidence suggests that the Sun was born near 5 kpc from the Galactic center, within the corotation radius of the Galactic bar, around 6-7 kpc. This presents challenge…

astro-ph.GA2024★ 2 cited

Chemical enrichment by collapsars as the origin of the unusually high [Ba/Fe] in a massive star cluster of the dwarf galaxy NGC 1569

Brayden Leicester, Kenji Bekki, Takuji Tsujimoto

The super star cluster NGC1569-B has recently been observed to have an extremely high [Ba/Fe]. We consider that the observed high [Ba/Fe] ( 1.3) is due to the chemical enrich…

astro-ph.HE2024★ 4 cited

Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background

Ken'ichiro Nakazato, Ryuichiro Akaho, Yosuke Ashida +1

Flux spectrum, event rate, and experimental sensitivity are investigated for the diffuse supernova neutrino background (DSNB), which originates from past stellar collapses and is a…

astro-ph.GA2024

Phosphorus enrichment by ONe novae in the Galaxy

Kenji Bekki, Takuji Tsujimoto

Recent observations have shown that [P/Fe] in the Galactic stars decreases with increasing [Fe/H] for [Fe/H] > -1 whereas it is almost subsolar for [Fe/H]< -2. These [P/Fe] trends…

astro-ph.GA2024

Joint r-Process Enrichment by Supernovae with a Metallicity Threshold and Neutron Star Mergers

Takuji Tsujimoto

The enrichment history of -process elements has been imprinted on the stellar abundances that change in accordance with increasing metallicity in galaxies. Close examination of…

astro-ph.GA2023

Exploring the Sun's birth radius and the distribution of planet building blocks in the Milky Way galaxy: A multi-zone Galactic chemical evolution approach

Junichi Baba, Takayuki R. Saitoh, Takuji Tsujimoto

We explore the influence of the Milky Way galaxy's chemical evolution on the formation, structure, and habitability of the Solar system. Using a multi-zone Galactic Chemical Evolut…

astro-ph.GA2011★ 9 cited

Implications of a non-universal IMF from C, N, and O abundances in very metal-poor Galactic stars and damped Lyman-alpha absorbers

T. Tsujimoto, K. Bekki

Recently revealed C, N, and O abundances in the most metal-poor damped Lyman-alpha (DLA) absorbers are compared with those of extremely metal-poor stars in the Galactic halo, as we…

astro-ph.GA2010★ 7 cited

Turn-off of Deuterium Astration in the Recent Star Formation of the Galaxy Disk

T. Tsujimoto

Chemical features of the local stellar disk have firmly established that long-term, continuous star formation has been accompanied by a steady rate of accretion of low-metallicity…

astro-ph1998★ 274 cited

Low-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution

Chiaki Kobayashi, Takuji Tsujimoto, Ken'ich Nomoto +2

We introduce a metallicity dependence of Type Ia supernova (SN Ia) rate into the Galactic and cosmic chemical evolution models. In our SN Ia progenitor scenario, the accreting whit…