Wind from T Tauri Stars

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 1998-12-01

著者

• KIGUCHI Masayoshi

  Research Institute for Science and Technology, Kinki University

• NARITA Shinji

  Science and Engineering Research Institute, Doshisha University

• Narita Shinji

  Science And Engineering Research Institute Doshisha University

• Hayashi C

  Kyoto University

• Narita S

  Science And Engineering Research Institute Doshisha University

• Kiguchi M

  Kinki Univ. Higashi‐osaka Jpn

• Kiguchi Masayoshi

  Research Institute For Fundamental Physics Kyoto University

• KIGUCHI Masayoshi

  Research Institute for Science and Technology Kinki University

関連論文

• The Formation of Molecules in Contracting Interstellar Clouds
• Primordial Solar Nebula Embedded in Corona
• Wind from T Tauri Stars
• The Structure and Evolution of Thin Viscous Disks-1-Non-steady Accretion and Excretion
• 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
• Fragmentation of Isothermal Sheet-Like Clouds. II : Full Nonlinear Numerical Simulations
• Fragmentation of Isothermal Sheet-Like Clouds. I : Solutions of Linear and Second-Order Perturbations Equation
• Characteristics of Collapse of Rotating Isothermal Clouds : Astrophysics and Relatively
• Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
• Adiabatic Collapse of Rotating Gas Clouds
• Fully Three-Dimensional Hydrodynamical Collapse and Formation of Binary System
• Hot Dense Matter and Stellar Collapse
• The Quantum Chromodynamic Black Body Radiation and the Universe
• Neutrino Cooling of Neutron Stars in Pion-Condensed Phase
• Excitation Energies in π-Electron Systems : Application of Green's Function Method with Second-Order Perturbaton Terms
• Characteristics of Collapse of Rotating Isothermal Clouds

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