Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
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関連論文
- 球状星団の形成と銀河の衝突史--マゼラン雲の歴史をたどる
- 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
- 大小マゼラン雲の衝突史とマゼラン電流(天文学の境界領域を探る,研究会報告)
- 銀河と宇宙の磁場
- Bisymmetric Spiral Configuration of Magnetic Fields in Spiral Galaxies-2-A Quasi-Global Theory
- 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
- 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
- 1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)
- Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
- Asymmetric Distribution of Gas in the Large Magellanic Cloud and Dynamical Condition for Globular Cluster Formation
- Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
- The Vertical Large-Scale Magnetic Fields in Spiral Galaxies
- 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
- Instability of Interaction Network for Interstellar Gas and Interstellar Diffusive Energy in the Shear Field
- An Upper Limit on the Mean Mass of Black Holes in the Galactic Halo
- Velocity Dispersion of Stars and Giant Molecular Clouds
- Numerical Simulation for Stellar Velocity Dispersion and Hardness of Encounters between Stars and Perturbers
- Dynamical Evolution of Galactic Disk Stars Due to Giant Molecular Clouds and Spiral Density Waves
- Dynamical Evolution of Galactic Disk Stars Due to Giant Molecular Clouds and Spiral Density Waves-2-
- Dynamics of Rotating Gaseous Ellipsoid in External Force Fields
- Characteristics of Collapse of Rotating Isothermal Clouds