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Tidal downsizing
Early Evolution of Clumps Formed Via Gravitational Instability in Protoplanetary Disks; Precursors of Hot Jupiters?
Pranav P Manangath Western University
Towards a Population Synthesis Model of Objects Formed by Self
Formation of Planets by Tidal Downsizing of Giant Planet Embryos
The Tidal Downsizing Hypothesis of Planet Formation
A New View on Planet Formation
Towards a Population Synthesis Model of Self-Gravitating Disc Fragmentation and Tidal Downsizing II: the Effect of Fragment–Fragment Interactions
Tidal Downsizing Model. II. Planet-Metallicity Correlations
Dawes Review. the Tidal Downsizing Hypothesis of Planet Formation
Dark Collapse of Gas Giant Planets
Rocky Planets Could Have Been Born As Gas Giants 16 September 2011, by Nola Taylor Redd
Tidal Downsizing Model. I. Numerical Methods: Saving Giant Planets from Tidal Disruptions
“Planet” to Refer to Objects with Mass Smaller Than ~13 M
Tidal Downsizing Model – I. Numerical Methods: Saving Giant Planets from Tidal Disruptions
Tidal Downsizing Model. III. Planets from Sub-Earths to Brown Dwarfs
Exploring the Conditions for Forming Cold Gas Giants Through Planetesimal Accretion Anders Johansen1 and Bertram Bitsch2
Tidal Downsizing Model – III. Planets from Sub-Earths to Brown Dwarfs: Structure and Metallicity Preferences
The Tidal Downsizing Hypothesis for Planet Formation and the Composition of Solar System Comets
Top View
Heavy Metal Rules. I. Exoplanet Incidence and Metallicity
IV. Destructive Feedback in Planets
Rotation of the Solar System Planets and the Origin of the Moon in the Context of the Tidal Downsizing Hypothesis