Shoken M. | National Astronomical Observatory
スポンサーリンク
概要
関連著者
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Shoken M.
National Astronomical Observatory
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Miyama Shoken
Department Of Physics Kyoto Univeristy
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Miyama Shoken
Department Of Physics Kyoto Unvi
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SEKIYA Minoru
Department of Applied Physics, Tokyo Institute of Technology
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Sekiya Minoru
Department Of Earth And Planetary Sciences Faculty Of Sciences 33 Kyushu University
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Sekiya Minoru
Department Of Applied Physics Tokyo Institute Of Technology
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SEKIYA Makoto
Department of Physics, Kyoto University
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SEKIYA Minoru
Department of Physics, Kyoto University
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SEKIYA Minoru
Department of Earth and Planetary Sciences, Faculty of Sciences 33, Kyushu University
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Miyama S
National Astronomical Observatory
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NARITA Shinji
Science and Engineering Research Institute, Doshisha University
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MIYAMA Shoken
National Astronomical Observatory
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Hayashi Chushiro
Kyoto University
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Narita Shinji
Department of Electronic Engineering, Doshisha University
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Narita Shinji
Science And Engineering Research Institute Doshisha University
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Hayashi C
Kyoto University
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Narita S
Science And Engineering Research Institute Doshisha University
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NARITA Shinji
Department of Electonics, Doshisha University
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KIGUCHI Masayoshi
Research Institute for Science and Technology, Kinki University
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Kiguchi M
Kinki Univ. Higashi‐osaka Jpn
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Kiguchi Masayoshi
Research Institute For Fundamental Physics Kyoto University
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NARITA Shinji
Department of Electronics, Doshisha University
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KIGUCHI Masayoshi
Research Institute for Science and Technology Kinki University
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TAKEDA Hidenori
Department of Physics, Kyoto University
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HAYASHI Chushiro
Department of Physics, Kyoto University
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Takeda Hidenori
Department Of Aeronautical Engineering Kyoto University
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Hidenori Takeda
Department Of Aeronautical Engineering Kyoto University
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Hayashi Chushiro
Department Of Nuclear Science Kyoto University
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Sekiya M
Department Of Mechanical And Precision System Teikyo University
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Sekiya Minoru
Department Of Earth And Planetary Sciences Kyushu University
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Kojima Yasuaki
Graduate School Of Engineering Hiroshima University
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KUBOTANI Hirto
Faculty of Engineering, Kanagawa University
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KOJIMA Yasufumi
Department of Physics, Tokyo Metropolitan University
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Kojima Y
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics University Of Wales
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KUBOTANI Hiroto
Department of Physics, Kyoto University
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藤本 光昭
名古屋市
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TAKEUCHI Taku
Department of Earth and Planetary Sciences, Faculty of Science, Tokyo Institute of Technology
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Takeuchi Taku
Department Of Earth And Planetary Sciences Faculty Of Science Tokyo Institute Of Technology
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Kubotani Hiroto
Department Of Mathenatics Nara University Of Education
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Kubotani Hiroto
Department Of Physics Kyoto University
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長沢 幹夫
(株)日立製作所
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TAKEDA Hidenori
Department of Aeronautics and Astronautics, Faculty of Engineering Kyoto University
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KOJIMA Yasufumi
Department of Physics, University of Wales
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SEKIYA Minoru
Department of Mechanical and Precision System, Teikyo University
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HAYASHI Chushiro
Department of Nuclear Science : Research Institute for Fundamental Physics Kyoto University : National Aeronautics and Space Administration
著作論文
- The Surface Wave Instability of Stratified Incompressible Cylinders with Differential Rotation : Astrophysics and Relativity
- Numerical Simulation of Viscous Flow by Smoothed Particle Hydrodynamics : Astrophysics and Relativity
- Chapter 23 Gas Capture by Proto-Jupiter and Proto-Saturn : Part VI Growth of the Planets : Origin of the Solar System
- Chapter 8 Efficiency of Angular Momentum Transfer by Shear Instability : Part II Formation Processes of Protostars : Origin of the Solar System
- Chapter 7 Stability of the Primordial Solar Nebula : Part II Formation Processes of Protostars : Origin of the Solar System
- Chapter 5 Collapse and Fragmentation of Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
- Chapter 4 The Equilibrium and the Stability of Rotating Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
- 1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)
- Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
- Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
- Wave Excitation in Isothermal Disks by External Gravity
- Criteria for the Collapse and Fragmentation of Rotating Clouds
- Three-Dimensional Hydrodynamical Simulations of Type 2 Supernova--Mixing and Fragmentation of Ejecta
- Time Evolution of Pure Gravitational Waves
- Characteristics of Collapse of Rotating Isothermal Clouds