スポンサーリンク
Department of Physics, Kyoto University | 論文
- 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
- 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
- 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
- Partially Connected Faddeev-Weinberg-Rosenberg Equation
- Theoretical Investigation on Induced Magnetic Moment by Impurity Potential
- Influence of α-Clustering on the Odd-Parity Levels in A=18 Nuclei
- Neural Network Model Carrying Phase Information with Application to Collective Dynamics : General and Mathematical Physics
- Transition Probability of Neutralization Process of +2 Ion Scatterd on a Metal Surface
- 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