スポンサーリンク
Department of Astronomy, School of Science, University of Tokyo | 論文
- 楕円銀河の高温ガスの熱源としてのIa型超新星(宇宙の階層構造,研究会報告)
- Modeling Dense Stellar Systems
- The Core Radius of a Star Cluster Containing a Massive Black Hole
- Infrared Camera (IRC) onboard ASTRO-F (IRIS)
- GreeM : Massively Parallel TreePM Code for Large Cosmological N-body Simulations
- Toward First-Principle Simulations of Galaxy Formation : II. Shock-Induced Starburst at a Collision Interface during the First Encounter of Interacting Galaxies
- Toward First-Principle Simulations of Galaxy Formation : I. How Should We Choose Star-Formation Criteria in High-Resolution Simulations of Disk Galaxies?
- Environmental Effect on the Subhalo Abundance : a Solution to the Missing Dwarf Problem
- BRIDGE : A Direct-Tree Hybrid N-Body Algorithm for Fully Self-Consistent Simulations of Star Clusters and Their Parent Galaxies
- Dynamical Friction on Satellite Galaxies
- GRAPE-6A : A Single-Card GRAPE-6 for Parallel PC-GRAPE Cluster Systems
- PGPG : An Automatic Generator of Pipeline Design for Programmable GRAPE Systems
- GRAPE-6A: A Single-Card GRAPE-6 for Parallel PC-GRAPE Cluster Systems
- A Fast Parallel Treecode with GRAPE
- PROGRAPE-1: A Programmable, Multi-Purpose Computer for Many-Body Simulations
- GRAPE Project : A Decade of Special-Purpose Computers for Many-Body Simulations
- Smoothing of the Anisotropy of the Cosmic Background Radiation by Multiple Gravitational Scattering
- The Evolution of Massive Black-Hole Binaries in Merging Galaxies-1-Evolution of a Binary in a Spherical Galaxy (GRAPE)
- Evolution of Clusters of Galaxies (GRAPE)
- Rapid Orbital Decay of a Black Hole Binary in Merging Galaxies