Environmental Effect on the Subhalo Abundance : a Solution to the Missing Dwarf Problem
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2008-08-25
著者
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MAKINO Junichiro
National Astronomical Observatory of Japan
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MAKINO Junichiro
Center for Computational Astrophysics, National Astronomical Observatory of Japan
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Makino Junichiro
Graduate Univ. Advanced Studies(sokendai) Tokyo
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ISHIYAMA Tomoaki
National Astronomical Observatory of Japan
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FUKUSHIGE Toshiyuki
Department of General System Studies, College of Arts and Sciences, The University of Tokyo
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Fukushige Toshiyuki
Univ. Tokyo Tokyo
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Fukushige Toshiyuki
Department Of General System Studies College Of Arts And Sciences The University Of Tokyo
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MAKINO Junichiro
Department of Astronomy, School of Science, University of Tokyo
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Fukushige Toshiyuki
Department of Earth Science and Astronomy, College of Arts and Sciences, The University of Tokyo
関連論文
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- 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
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- 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
- Energy Segregation through Violent Relaxation
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- DREAM--A Special-Purpose Computer for Large Scale Mesh Calculations
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- PPPM and TreePM Methods on GRAPE Systems for Cosmological N-Body Simulations
- Mass-Loss Timescale of Star Clusters in an External Tidal Field : II. Effect of Mass Profile of Parent Galaxy
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- Gravothermal Expansion in N-Body Systems