KOKUBO Eiichiro | Center for Computational Astrophysics, National Astronomical Observatory of Japan
スポンサーリンク
概要
関連著者
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台坂博
一橋大学
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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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KOKUBO Eiichiro
The Graduate University for Advanced Studies
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Saitoh Takayuki
Center For Computational Astrophysics National Astronomical Observatory Of Japan
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Yoshida Naoki
Institute For The Physics And Mathematics Of The Universe The University Of Tokyo
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Makino Junichiro
Graduate Univ. Advanced Studies(sokendai) Tokyo
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Tomisaka Kohji
Center For Computational Astrophysics National Astronomical Observatory Of Japan
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DAISAKA Hiroshi
Graduate School of Commerce and Management, Hitotsubashi University
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KOKUBO Eiichiro
Center for Computational Astrophysics, National Astronomical Observatory of Japan
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OKAMOTO Takashi
Institute for Computational Cosmology, Department of Physics, Durham University
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WADA Keiichi
Center for Computational Astrophysics, National Astronomical Observatory of Japan
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Wada Keiichi
Kagoshima Univ. Kagoshima
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台坂 博
Graduate School Of Commerce And Management Hitotsubashi University
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Makino Junichiro
Center For Computational Astrophysics National Astronomical Observatory Of Japan
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Okamoto Takashi
Institute For Computational Cosmology Department Of Physics Durham University
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Saitoh Takayuki
National Astronomical Observatory Of Japan Tokyo
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MAKINO Junichiro
Department of Astronomy, School of Science, University of Tokyo
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YOSHIDA Naoki
Department of Cardiology, Nagoya University Graduate School of Medicine
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Yoshida Naoki
Department Of Cardiology Nagoya University Graduate School Of Medicine
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Yoshida Naoki
Institute For Materials Research Tohoku University
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YOSHIDA Naoki
Department of Biomolecular Engineering, Tohoku University
著作論文
- 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?