Were planetesimals formed by dust accretion in the solar nebula?

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Chapter II Evolution of the Expanding Hot Universe
On the Dissipation of Primordial Turbulence in the Expanding Universe
Galaxy Formation and the Primordial Turbulence in the Expanding Hot Universe
Cooling of Pre-Galactic Gas Clouds by Hydrogen Molecule
Cooling of Pre-Galactic Gas Clouds by Hydrogen Molecule
Formation of H_2 and Galaxies in the Hot Universe
Gas Drag on a Rotating Body with Gravity
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?
On the Acoustic Decay of Primordial Cosmic Turbulence
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
Flows in a Rotating Cylinder with a Sloping Bottom
Non-axisymmetric flow in a rotating cylinder : Incompressible and compressible fluids
Drag on a Gravitating Sphere Moving through a Gas : Astrophysics and Relativity
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
Time Variation of Metal Abundance in Galaxies : Super-Metal-Rich Stage
Dissipation of Primordial Turbulence and Thermal History of the Universe
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
The Sound Generated by Cosmic Turbulence and the Origin of Galaxies
Chapter 17 Drag on a Gravitating Body : Part V Physical Processes Relevant to the Planetary Growth : Origin of the Solar System
Thermal evolution of icy planetesimals in the solar nebula

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