Nakano Takenori | Research Institute For Fundamental Physics Kyoto University

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概要

• 同名の論文著者
• Research Institute For Fundamental Physics Kyoto Universityの論文著者

関連著者

• Hayashi Chushiro

  Department Of Nuclear Science Kyoto University

• Nakano Takenori

  Research Institute For Fundamental Physics Kyoto University

• HAYASHI Chushiro

  Department of Nuclear Science : Research Institute for Fundamental Physics Kyoto University : National Aeronautics and Space Administration

• HAYASHI Chushiro

  Department of Physics, Kyoto University

• Narita Shinji

  Department of Electronic Engineering, Doshisha University

• Narita Shinji

  Department Of Physics Kyoto University

• NAKANO Takenori

  Research Institute for Fundamental Physics, Kyoto University

• Nakano Takenori

  Research Institute For Fundamental Physics Kyoto University : National Radio Astronomy Observatory

• Kusaka Takashi

  Department Of Biochemistry Kawasaki Medical School

• Ohyama Noboru

  Department Of Nuclear Science Kyoto University

• Ohyama Noboru

  Department Of Physics Hiroshima University

• Ohyama Noboru

  Faculty Of Engineering Shizuoka University

• Nakano Takenori

  Research Institute For Fundamental Physics Kyoto University : National Radio Astronomy Observatory C

• HATTORI Tsuguo

  Department of Physics, Kyoto University

• Kusaka Takashi

  Department Of Physics Kyoto University

• Hattori Tsuguo

  Department Of Physics Kyoto University

• KUSAKA Takashi

  Department of Physics, Kyoto University

• NARITA Shinji

  Department of Electonics, Doshisha University

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著作論文

• Rapid Contraction of Protostars to the Stage of Quasi-Hydrostatic Equilibrium. III : Stars of 0.05, 1.0 and 20Mxodoi with Energy Flow by Radiation and Convection
• Collapse and Flare-up of Protostars
• Thermal and Dynamical Evolution of Gas Clouds of Various Masses
• Rapid Contraction of Protostars to the Stage of Quasi-Hydrostatic Equilibrium. II : 10, 10^2, 10^3 and 10^4 Solar Masses without Radiation Flow
• Rapid Contraction of a Protostar to the Stage of Quasi-Hydrostatic Equilibrium. I : The Case of One Solar Mass without Radiation Flow
• Growth of Solid Particles in the Primordial Solar Nebula

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