Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
スポンサーリンク
概要
- 論文の詳細を見る
- 理論物理学刊行会の論文
- 1982-12-25
著者
-
HAYASHI Chushiro
Department of Physics, Kyoto University
-
Miyama S
National Astronomical Observatory
-
Miyama Shoken
Department Of Physics Kyoto Unvi
-
Miyama Shoken
Department Of Physics Kyoto Univeristy
-
Hayashi Chushiro
Department Of Nuclear Science Kyoto University
-
NARITA Shinji
Science and Engineering Research Institute, Doshisha University
-
Narita Shinji
Department of Electronic Engineering, Doshisha University
-
Shoken M.
National Astronomical Observatory
-
Narita Shinji
Science And Engineering Research Institute Doshisha University
-
Hayashi C
Kyoto University
-
Narita S
Science And Engineering Research Institute Doshisha University
-
NARITA Shinji
Department of Electronics, Doshisha University
-
NARITA Shinji
Department of Electonics, Doshisha University
-
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
- Primordial Solar Nebula Embedded in Corona
- 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
- The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula
- Wind from T Tauri Stars
- The Structure and Evolution of Thin Viscous Disks-1-Non-steady Accretion and Excretion
- 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
- 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
- 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
- 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
- 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
- 1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)
- 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
- Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
- 3次元自己重力系における構造発生(基研短期研究会『天体現象と非線形・非平衡物理』報告,研究会報告)
- 3-D Numerical Hydrodynamics of Self-Gravitating Gas : Collisions and Fragmentations
- Three-Dimensional Numerical Simulation of Interstellar Cloud-Cloud Collisions and Triggered Star Formation. I : Head-On Collisions
- Adiabatic Collapse of Rotating Gas Clouds
- Isothermal Collapse of Rotating Gas Clouds
- Thermal and Dynamical Evolution of Gas Clouds of Various Masses
- The Radiative Energy Loss from the Shock Front
- Fully Three-Dimensional Hydrodynamical Collapse and Formation of Binary System
- Helium Capturing Reactions in Stars
- ポリトロープ星の三次元爆発(基研短期研究会「SN1987A」,研究会報告)
- 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
- Fragmentation of Clouds(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation)
- Evolution of Carbon Stars. II : Carbon Burning Phase
- Is the Conventional Big Bang Compatible with the Discovery of the Quarks?
- An Upper Bound on the Number Density of Primordial Black Holes from the Big Bang Nucleosynthesis
- 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
- General Relativistic Collapse of an Axially Symmetric Star. I : The Formulation and the Initial Value Equations
- A Method of Determining Apparent Horizons in [(2+1)+1]-Formalism of the Einstein Equations
- An Analytic Solution of Initial Data for Slowly Rotating Dust Sphere under Maximal Slicing Condition
- A New Formalism of the Einstein Equations for Relativisitic Rotating Systems
- Instability of a Gaseous Envelope Surrounding a Planetary Core and Formation of Giant Planets
- The Evolution of Massive Stars. I
- Excitation Energies in π-Electron Systems : Application of Green's Function Method with Second-Order Perturbaton Terms
- The Catalysis of Nuclear Fusion Reactions by μ^--Mesons
- Constraints on Lifetime and Mass of Heavy Lepton Neutrinos Imposed by Big Bang Nucleosynthesis
- Evolution of a Star with Intermediate Mass after Hydrogen Burning
- Formation of Light Nuclei in the Expanding Universe
- Internal Structure of Very Massive Stars
- Characteristics of Collapse of Rotating Isothermal Clouds
- Hamiltonian Formalism in Non-local Field Theories