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20042026
most citedA Necessary Condition for Individual Time-Steps in SPH Simulations

194 citations · 2.5k across the 56 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

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.IM2016★ 71 cited

Chemical evolution library for galaxy formation simulation

Takayuki R. Saitoh

We have developed a software library for chemical evolution simulations of galaxy formation under the simple stellar population (SSP) approximation. In this library, all of the nec…

astro-ph.GA2016★ 42 cited

Eventful Evolution of Giant Molecular Clouds in Dynamically Evolving Spiral Arms

Junichi Baba, Kana Morokuma-Matsui, Takayuki R. Saitoh

The formation and evolution of giant molecular clouds (GMCs) in spiral galaxies have been investigated in the traditional framework of the combined quasi-stationary density wave an…

astro-ph.GA2016★ 20 cited

Santa Barbara Cluster Comparison Test with DISPH

Takayuki Saitoh, Junichiro Makino

The Santa Barbara cluster comparison project (Frenk et al. Frenk+1999) revealed that there is a systematic difference between entropy profiles of clusters of galaxies obtained by E…

astro-ph.IM2016★ 19 cited

A comparison of SPH artificial viscosities and their impact on the Keplerian disk

Natsuki Hosono, Takayuki R. Saitoh, Junichiro Makino

Hydrodynamical simulations of rotating disk play important roles in the field of astrophysical and planetary science. Smoothed Particle Hydrodynamics (SPH) has been widely used for…

astro-ph.EP2016★ 3 cited

The Giant Impact Simulations with Density Independent Smoothed Particle Hydrodynamics

Natsuki Hosono, Takayuki R. Saitoh, Junichiro Makino +2

At present, the giant impact (GI) is the most widely accepted model for the origin of the Moon. Most of the numerical simulations of GI have been carried out with the smoothed part…