activity
19962018
most citedNeutron-capture elements in the very metal-poor star HD122563

229 citations · 1.6k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2018★ 42 cited

Stochastic Chemical Evolution of Galactic Subhalos and the Origin of r-Process Elements

Takuya Ojima, Yuhri Ishimaru, Shinya Wanajo +2

Mergers of compact binaries (of a neutron star and another neutron star or a black hole, NSMs) are suggested to be the promising astrophysical site of the r-process. While the aver…

astro-ph.GA2018★ 43 cited

Enrichment of Zinc in galactic chemodynamical evolution models

Yutaka Hirai, Takayuki R. Saitoh, Yuhri Ishimaru +1

The heaviest iron-peak element, Zn has been used as an important tracer of cosmic chemical evolution. Spectroscopic observations of the metal-poor stars in Local Group galaxies sho…

astro-ph.SR2017★ 27 cited

Diversity of Abundance Patterns of Light Neutron-capture Elements in Very-metal-poor Stars

Misa Aoki, Yuhri Ishimaru, Wako Aoki +1

We determine the abundances of neutron-capture elements from Sr to Eu for five very-metal-poor stars (-3<[Fe/H]<-2) in the Milky Way halo to reveal the origin of light neutron-capt…

astro-ph.GA2016★ 40 cited

Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements

Yutaka Hirai, Yuhri Ishimaru, Takayuki R. Saitoh +3

The abundance of elements synthesized by the rapid neutron-capture process (r-process elements) of extremely metal-poor (EMP) stars in the Local Group galaxies gives us clues to cl…

astro-ph.GA2015★ 113 cited

Enrichment of r-process elements in dwarf spheroidal galaxies in chemo-dynamical evolution model

Yutaka Hirai, Yuhri Ishimaru, Takayuki R. Saitoh +3

The rapid neutron-capture process (r-process) is a major process to synthesize elements heavier than iron, but the astrophysical site(s) of r-process is not identified yet. Neutron…

astro-ph.GA2015★ 108 cited

Neutron Star Mergers as the Origin of r-Process Elements in the Galactic Halo Based on the Sub-halo Clustering Scenario

Yuhri Ishimaru, Shinya Wanajo, Nikos Prantzos

Binary mergers (NSMs) of double neutron star (and black hole-neutron star) systems are suggested to be major sites of r-process elements in the Galaxy by recent hydrodynamical and…