Shear instabilities in the dust layer of the solar nebula II. Different unperturbed states
スポンサーリンク
概要
著者
-
Ishitsu Naoki
Department Of Earth And Planetary Sciences Graduate School Of Sciences 33 Kyushu University
-
Ishitsu Naoki
Department Of Earth And Planetaly Sciences Graduate School Of Sciences Kyushu University
-
Sekiya Minoru
Department Of Earth And Planetary Sciences Faculty Of Sciences 33 Kyushu University
-
Sekiya Minoru
Department Of Applied Physics Tokyo Institute Of Technology
-
Sekiya Minoru
Department of Earth and Planetary Sciences, Faculty of Sciences, 33 Kyushu University
関連論文
- Chapter 12 Settling of Dust Particles and Formation of Planetesimals : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
- Cosmic-ray exposure age and heliocentric distance of the parent body of H chondrites Yamato-75029 and Tsukuba
- Collisional destruction experiment of chondrules and formation of fragments in the solar nebula
- Formation processes of magnetic spherules collected from deep-sea sediments -Observations and numerical simulations of the orbital evolution-
- 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
- Were planetesimals formed by dust accretion in the solar nebula?
- 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
- Flow in a Liquid Sphere Moving with a Hypersonic Velocity in a Rarefied Gas : An Analytic Solution of Linearized Equations
- Gravitational Instabilities in a Dust-Gas Layer and Formation of Planetesimals in the Solar Nebula
- 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
- Deformation and internal flow of a chondrule-precursor molten sphere in a shocked nebular gas
- Flow in a Liquid Sphere Moving with a Hypersonic Velocity in a Rarefied Gas : An Analytic Solution of Linearized Equations
- Shear instabilities in the dust layer of the solar nebula II. Different unperturbed states
- Shear instabilities in the dust layer of the solar nebula I. The linear analysis of a non-gravitating one-fluid model without the Coriolis and the solar tidal forces
- On the Peculiarity of the Pion in the Composite Model of Hadrons
- The Generalized Dual Loop Expansion of U(N_c) Gauge Theory
- Shear instabilities in the dust layer of the solar nebula III. Effects of the Coriolis force
- Condition for the formation of the compound chondrules in the solar nebula
- Thermal evolution of icy planetesimals in the solar nebula