Search Results - "SAITOH, R"
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A DENSITY-INDEPENDENT FORMULATION OF SMOOTHED PARTICLE HYDRODYNAMICS
Published in The Astrophysical journal (01-05-2013)“…The standard formulation of the smoothed particle hydrodynamics (SPH) assumes that the local density distribution is differentiable. This assumption is used to…”
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SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
Published in Publications of the Astronomical Society of Japan (01-08-2021)“…Abstract Most stars are formed as star clusters in galaxies, which then disperse into galactic disks. Upcoming exascale supercomputational facilities will…”
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Eventful evolution of giant molecular clouds in dynamically evolving spiral arms
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…The formation and evolution of giant molecular clouds (GMCs) in spiral galaxies have been investigated in the traditional framework of the combined…”
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Natures of a clump-origin bulge: a pseudo-bulge like but old metal-rich bulge
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…Bulges in spiral galaxies have been supposed to be classified into classical bulges or pseudo-bulges. Classical bulges are thought to form by galactic merger…”
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Compact Object Mergers Driven by Gas Fallback
Published in Physical review letters (29-06-2018)“…Recently, several gravitational wave detections have shown evidence for compact object mergers. However, the astrophysical origin of merging binaries is not…”
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SIRIUS project. II. A new tree-direct hybrid code for smoothed particle hydrodynamics/ N -body simulations of star clusters
Published in Publications of the Astronomical Society of Japan (01-08-2021)“…Abstract Star clusters form via clustering star formation inside molecular clouds. In order to understand the dynamical evolution of star clusters in their…”
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Enrichment of Zinc in Galactic Chemodynamical Evolution Models
Published in The Astrophysical journal (01-03-2018)“…The heaviest iron-peak element Zinc (Zn) has been used as an important tracer of cosmic chemical evolution. Spectroscopic observations of the metal-poor stars…”
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Origin of highly r -process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
Published in Monthly notices of the Royal Astronomical Society (14-11-2022)“…ABSTRACT The r-process-enhanced (RPE) stars provide fossil records of the assembly history of the Milky Way (MW) and the nucleosynthesis of the heaviest…”
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THE FORMATION OF YOUNG DENSE STAR CLUSTERS THROUGH MERGERS
Published in The Astrophysical journal (01-07-2012)“…Young star clusters such as NGC 3603 and Westerlund 1 and 2 in the Milky Way and R136 in the Large Magellanic Cloud are dynamically more evolved than expected…”
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Chemo-dynamical Evolution of Simulated Satellites for a Milky Way–like Galaxy
Published in The Astrophysical journal (01-08-2024)“…Abstract The chemical abundances of Milky Way’s (MW's) satellites reflect their star formation histories (SFHs), yet, due to the difficulty of determining the…”
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Property of young massive clusters in a galaxy–galaxy merger remnant
Published in Publications of the Astronomical Society of Japan (01-01-2019)“…Abstract We investigate the properties of young massive clusters (YMCs) in a galaxy–galaxy merger remnant by analyzing the data obtained by a gas-rich major…”
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On the Interpretation of the l–v Features in the Milky Way Galaxy
Published in Publications of the Astronomical Society of Japan (25-12-2010)“…We modeled the gas dynamics of barred galaxies using a three-dimensional, high-resolution, $N$ -body $+$ hydrodynamical simulation, and applied it to the Milky…”
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Massive first star binaries as new tools for Galactic archaeology
Published in EPJ Web of conferences (01-01-2022)“…Binary systems are important probes of the origin of stars with peculiar chemical features through the interactions between two stars. We have studied the…”
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DYNAMICS OF NON-STEADY SPIRAL ARMS IN DISK GALAXIES
Published in The Astrophysical journal (20-01-2013)“…In order to understand the physical mechanisms underlying non-steady stellar spiral arms in disk galaxies, we analyzed the growing and damping phases of their…”
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Tidal Disruption of Dark Matter Halos around Proto-Globular Clusters
Published in The Astrophysical journal (20-03-2006)“…Tidal disruption of dark matter halos around proto-globular clusters in the halo of a small galaxy is studied in the context of the hierarchical clustering…”
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Exploring the Sun’s birth radius and the distribution of planet building blocks in the Milky Way galaxy: a multizone Galactic chemical evolution approach
Published in Monthly notices of the Royal Astronomical Society (20-10-2023)“…ABSTRACT We explore the influence of the Milky Way galaxy’s chemical evolution on the formation, structure, and habitability of the Solar system. Using a…”
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Interplay between Stellar Spirals and the Interstellar Medium in Galactic Disks
Published in The Astrophysical journal (01-07-2011)“…We propose a new dynamical picture of galactic stellar and gas spirals, based on hydrodynamic simulations in a 'live' stellar disk. We focus especially on…”
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Imprints of zero-age velocity dispersions and dynamical heating on the age–velocity dispersion relation
Published in Publications of the Astronomical Society of Japan (01-04-2017)“…Abstract Observations of stars in the the solar vicinity show a clear tendency of old stars to have larger velocity dispersions. This relation is called the…”
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Enrichment of Strontium in Dwarf Galaxies
Published in The Astrophysical journal (01-11-2019)“…Light trans-iron elements such as Sr serve as the key to understanding the astrophysical sites of heavy elements. Spectroscopic studies of metal-poor stars…”
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A Necessary Condition for Individual Time Steps in SPH Simulations
Published in The Astrophysical journal (01-06-2009)Get full text
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