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Alessandro Trani
The Astrophysical Journal, 2016
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Formation of the saturnian system: A modern Laplacian theory
Andrew Prentice
Earth, Moon and Planets, 1984
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The formation of planetary systems: from the ISM to planets
Ana I Gomez de Castro
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Eccentric disc instability in stellar discs formed from inspiralling gas clouds in the Galactic Centre
Hagai Perets
Monthly Notices of the Royal Astronomical Society, 2012
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The Origin of the Local System of Gas and Stars
carlos olano
The Astronomical Journal, 2001
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A gas-kinetic stability analysis of self-gravitating and collisional particulate disks with application to Saturn’s rings
Michael Gedalin
Planetary and Space Science, 2000
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The kinematics of gas and stars in the solar neighbourhood
Thomas Goulet
1984
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Thermohydrodynamics of Circumstellar Disks with High-Mass Planets
Gennaro D'Angelo, Wilhelm Kley
Astrophysical Journal, 2003
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Formation and evolution of planetary systems: Upper limits to the gas mass in disks around sun-like stars
Jinyoung Kim
2008
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Structure and evolution of circumstellar disks during the early phase of accretion from a parent cloud
olusola idowu
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Sharp eccentric rings in planetless hydrodynamical models of debris disks
W. Lyra
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Solar System. Angular Momentum. New Physics
Vladimir Netchitailo
JHEPGC, 2019
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The dynamics of Jupiter and Saturn in the gaseous protoplanetary disk
A. Crida
Icarus, 2007
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Formation of sharp eccentric rings in debris disks with gas but without planets
W. Lyra
Nature, 2013
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Circumplanetary Disk Formation
Robin Canup
The Astronomical Journal, 2010
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On The Origin of The High-Perihelion Scattered Disk: The Role of The Kozai Mechanism And Mean Motion Resonances
ADRIAN GALLARDO
Celestial Mechanics & Dynamical Astronomy, 2005
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Accretion of terrestrial planets from oligarchs in a turbulent disk
Shigeru Ida
Icarus, 2007
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Formation, orbital and thermal evolution, and survival of planetary-mass clumps in the early phase of circumstellar disc evolution
Shu-ichiro Inutsuka
Monthly Notices of the Royal Astronomical Society, 2013
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The role of particle collisions for the dynamics in planetary rings
Nikolai Brilliantov
Chaos, Solitons & Fractals, 1995
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The Self-gravitating Gas Fraction and the Critical Density for Star Formation
Blakesley Burkhart
The Astrophysical Journal, 2019
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Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture
A. Crida
The Astronomical Journal, 2007
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Preprint typeset using LATEX style emulateapj v. 11/10/09 TWO-COMPONENT SECULAR GRAVITATIONAL INSTABILITY IN A PROTOPLANETARY DISK: A POSSIBLE MECHANISM FOR CREATING RING-LIKE STRUCTURES
Shu-ichiro Inutsuka
2014
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Fluid Dynamic Aspects of Protostellar Disks Formation
Gérard Capitaine
The Astrophysical Journal 877:126, 2019
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Inner resonance ring of NGC 3081, disk surface mass density, and the enhanced disk few-body process
Tarsh Freeman, Gene Byrd
2006
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REMNANT GAS IN EVOLVED CIRCUMSTELLAR DISKS: HERSCHEL PACS OBSERVATIONS of 10-100 Myr OLD DISK SYSTEMS
Arnold Benz
The Astrophysical Journal, 2012
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Gravitational accretion of particles in Saturn's rings
R. Karjalainen
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Warm Molecular Gas Traced with CO J = 7 ! 6 in the Galaxy's Central 2 pc: Dynamical Heating of the Circumnuclear Disk
Maureen Savage
Astrophys J, 2005
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Nebular gas drag and planetary accretion with eccentric high-mass planets
Thierry Chanut
Astronomy & Astrophysics, 2013
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Statistical Mechanics and Dynamics of the Outer Solar System: II. The Saturn/Uranus and Uranus/Neptune Zones
Kevin William
1997
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Thermal forces on planetary ring particles: application to the main system of Saturn
David Nesvorný
Astronomy and Astrophysics, 2007
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Kinematics of gas and stars in the circumnuclear star-forming ring of NGC 3351
Ángeles Díaz
Monthly Notices of the Royal Astronomical Society, 2007
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Circum-planetary discs as bottlenecks for gas accretion onto giant planets
A. Crida
Astronomy & Astrophysics, 2012
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The Dynamical Evolution of the Circumstellar Gas around Low‐ and Intermediate‐Mass Stars. I. The Asymptotic Giant Branch
Arturo Manchado
The Astrophysical Journal, 2002
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EPEMC :: Opinion Editorial Haumea Ring Destroys Accretion Model Why the Accretion Model (AM) is inadequate for ring formation, as demonstrated by Haumea; favoring the electromagnetic Coalescence Model
Shifu Careaga
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Formation Process of the Circumstellar Disk: Long-term Simulations in the Main Accretion Phase of Star Formation
Shu-ichiro Inutsuka
2010
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