Evolution of the Stars
スポンサーリンク
概要
著者
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HAYASHI Chushiro
Department of Physics, Kyoto University
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SUGIMOTO Daiichiro
Department of Earth Science and Astronomy College of General Education, University of Tokyo
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Hayashi Chushiro
Department Of Nuclear Science Kyoto University
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HOSHI Reun
Department of Nuclear Science, Kyoto University
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Hoshi Reun
Department Of Nuclear Science Kyoto University
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Sugimoto Daiichiro
Department Of Earth Science And Astronomy College Of General Education University Of Tokyo
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SUGIMOTO Daiichiro
Department of Nuclear Science, Kyoto University
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HAYASHI Chushiro
Department of Nuclear Science : Research Institute for Fundamental Physics Kyoto University : National Aeronautics and Space Administration
関連論文
- Size Distribution of Grains Growing by Thermal Grain-Grain Collision
- Gravothermal Catastrophe and Negative Specific Heat of Self-Gravitating Systems
- Rapidly Rotating Polytropes and Concave Hamburger Equilibrium
- Dumb-Bell-Shape Equilibria and Mass-Shedding Pear-Shape of Selfgravitating Incompressible Fluid
- Gravothermal Aspects in Evolution of the Stars and the Universe
- Thermal Properties of Self-Gravitating Plane-Symmetric Configuration
- The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula
- The PCI Interface for GRAPE Systems : PCI-HIB
- Dissipation of the Primordial Terrestrial Atmosphere Due to lrradiation of the Solar Far-UV during T Tauri Stage
- Dissipation of the Primordial Terrestrial Atmosphere Due to irradiation of the Solar EUV
- Stellar Evolution toward Pre-Supernova Stage. II : Carbon and Oxygen Stars of 1.5Mxodoi and 2.6Mxodoi
- Effect of Electron Capture on the Temperature in Dense Stars
- Evolution of Iron Stars : Gravitational Contraction and the Decomposition of Iron
- Stable Numerical Method in Computation of Stellar Evolution
- Proton-Neutron Concentration Ratio in the Expanding Universe at the Stages preceding the Formation of the Elements
- Stellar Synthesis of the α-Particle Nuclei Heavier than Ne^
- Rapid Thermonuclear Reactions in Supernova Explosion
- Another Equilibrium Sequence of Self-Gravitating and Rotating Incompressible Fluid
- Giant Stars with Shell Sources of C-N and p-p Reactions
- Thermal and Dynamical Properties of a Protostar and Its Contraction to the Stage of Quasi-Static Equilibrium
- Proton-Neutron Concentration Ratio in the Expanding Universe at the Stages preceding the Formation of the Elements.
- Central Temperature and Density of Stars in Gravitational Equilibrium
- Evolution of the Stars
- Formation of the Planets
- 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
- Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
- Adiabatic Collapse of Rotating Gas Clouds
- Isothermal Collapse of Rotating Gas Clouds
- Thermal and Dynamical Evolution of Gas Clouds of Various Masses
- Helium Capturing Reactions in Stars
- Evolution of Carbon Stars. II : Carbon Burning Phase
- 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
- Contraction of a Protostar up to the Stage of Quasi-Static Equilibrium
- 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
- Evolution of Carbon Stars. I : Gravitational Contraction and Onset of Carbon Burning
- Advanced Phases of Evolution of Population II Stars : Growth of the Carbon Core and Shell Helium Flashes
- Stellar Evolution toward Pre-Supernova Stage. I : Carbon and Oxygen Stars of 5M_&odoi;, 10M_&odoi; and 30M_&odoi;
- Evolution of Massive Stars. II : Helium-Burning Stage
- Instability of a Gaseous Envelope Surrounding a Planetary Core and Formation of Giant Planets
- The Evolution of Massive Stars. I
- The Catalysis of Nuclear Fusion Reactions by μ^--Mesons
- Mixing between Stellar Envelope and Core in Advanced Phases of Evolution. I : General Treatment and Brief Summary of Results
- Evolution of a Star with Intermediate Mass after Hydrogen Burning
- Evolution of Population II Stars in the Helium-Burning Phase
- Formation of Light Nuclei in the Expanding Universe
- Concave Hamburger Equilibrium of Rotating Bodies
- Second Helium Flash and an Origin of Carbon Stars
- Helium Flash in Less Massive Stars
- Internal Structure of Very Massive Stars
- An Energetics of Quasar
- Hamiltonian Formalism in Non-local Field Theories