activity
20082026
most citedThe Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars

436 citations · 860 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Abundance analysis of three new extremely metal-poor stars, including one CEMP-s star

P. François, T. Suda, S. Wanajo +5

We report a detailed abundance analysis of three extremely metal-poor (EMP) stars thanks to spectra obtained with the high-dispersion spectrograph (HDS) at the Subaru telescope. Th…

astro-ph.SR2023

A comparative study on three modes of s-process nucleosynthesis in extremely metal-poor AGB stars

S. Yamada, T. Suada, Y. Komiya +2

Carbon-enhanced metal-poor (CEMP) stars in the Galactic halo have a wide range of neutron-capture element abundance patterns. To identify their origin, we investigated three modes…

astro-ph.SR2020★ 21 cited

Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?

Yutaka Komiya, Takuma Suda, Shimako Yamada +1

Mixing and fallback models in faint supernova models are supposed to reproduce the abundance patterns of observed carbon-enhanced metal-poor (CEMP) stars in the Galactic halo. A fi…

astro-ph.GA2017★ 95 cited

Stellar Abundances for Galactic Archaeology Database IV - Compilation of Stars in Dwarf Galaxies

Takuma Suda, Jun Hidaka, Wako Aoki +7

We have constructed the database of stars in the local group using the extended version of the SAGA (Stellar Abundances for Galactic Archaeology) database that contains stars in 24…

astro-ph.SR2016★ 1 cited

The s-Process Nucleosynthesis in Extremely Metal-Poor Stars as the Generating Mechanism of Carbon Enhanced Metal-Poor Stars

Takuma Suda, Shimako Yamada, Masayuki Y. Fujimoto

The origin of carbon-enhanced metal-poor (CEMP) stars plays a key role in characterising the formation and evolution of the first stars and the Galaxy since the extremely-poor (EMP…

astro-ph.GA2014★ 54 cited

The New Model of Chemical Evolution of r-process Elements Based on The Hierarchical Galaxy Formation I: Ba and Eu

Yutaka Komiya, Shimako Yamada, Takuma Suda +1

We investigate the chemical enrichment of r-process elements in the early evolutionary stages of the Milky Way halo within the framework of hierarchical galaxy formation using a se…

astro-ph.GA2013★ 84 cited

The Stellar Abundances for Galactic Archaeology (SAGA) Database III - Analysis of Enrichment Histories for Elements and Two Modes of Star Formation during the Early Evolution of Milky Way

Shimako Yamada, Takuma Suda, Yutaka Komiya +2

We study the enrichment histories for nine elements, C, four alpha-elements of Mg, Si, Ca, and Ti, Sc, and three iron-peak elements of Co, Ni, and Zn, by using a large number of st…

astro-ph.GA2013★ 47 cited

Transition of the Stellar Initial Mass Function Explored with Binary Population Synthesis

Takuma Suda, Yutaka Komiya, Shimako Yamada +7

The stellar initial mass function (IMF) plays a crucial role in determining the number of surviving stars in galaxies, the chemical composition of the interstellar medium, and the…

astro-ph.GA2010★ 117 cited

The Stellar Abundances for Galactic Archaeology (SAGA) Database II - Implications for Mixing and Nucleosynthesis in Extremely Metal-Poor Stars and Chemical Enrichment of the Galaxy

Takuma Suda, Shimako Yamada, Yutaka Katsuta +4

We discuss the characteristics of known extremely metal-poor (EMP) stars in the Galaxy using the Stellar Abundances for Galactic Archaeology (SAGA) database (Suda et al. 2008, PASJ…

astro-ph2008★ 436 cited

The Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars

Takuma Suda, Yutaka Katsuta, Shimako Yamada +6

We describe the construction of a database of extremely metal-poor (EMP) stars in the Galactic halo whose elemental abundances have been determined. Our database contains detailed…

astro-ph2008★ 5 cited

Tidal Interactions of Red Giants with Environment Stars in Globular Clusters

Shimako Yamada, Atsuo T. Okazaki, Masayuki Y. Fujimoto

We investigate the tidal interactions of a red giant with a main sequence in the dense stellar core of globular clusters by Smoothed Particle Hydrodynamics method. Two models of $0…