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Cited article:

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Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?

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Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses

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Astronomy & Astrophysics 644 A174 (2020)
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Giant planet formation at the pressure maxima of protoplanetary disks

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Dynamical Gaseous Rings in Global Simulations of Protoplanetary Disk Formation

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3D simulations of planet trapping at disc–cavity boundaries

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The Impact of Accretion Heating and Thermal Conduction on the Dead Zone of Protoplanetary Disks

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Thermal torque effects on the migration of growing low-mass planets

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Formation of Solar system analogues – II. Post-gas-phase growthand water accretion in extended discs via N-body simulations

M P Ronco and G C de Elía
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The Complex Morphology of the Young Disk MWC 758: Spirals and Dust Clumps around a Large Cavity

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