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Model of a Gap Formed by a Planet with Fast Inward Migration

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The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario

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Theoretical versus Observational Uncertainties: Composition of Giant Exoplanets

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Giant planet formation at the pressure maxima of protoplanetary disks

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Influence of migration models and thermal torque on planetary growth in the pebble accretion scenario

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Influence of sub- and super-solar metallicities on the composition of solid planetary building blocks

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Astronomy & Astrophysics 633 A10 (2020)
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Impact of vertical gas accretion on the carbon-to-oxygen ratio of gas giant atmospheres

Alexander J. Cridland, Arthur D. Bosman and Ewine F. van Dishoeck
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The Preservation of Super-Earths and the Emergence of Gas Giants after Their Progenitor Cores Have Entered the Pebble-isolation Phase

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The Astrophysical Journal 896 (2) 135 (2020)
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Thermal torque effects on the migration of growing low-mass planets

O M Guilera, N Cuello, M Montesinos, et al.
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Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion, and disc evolution

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Vortex instabilities triggered by low-mass planets in pebble-rich, inviscid protoplanetary discs

A Pierens, M-K Lin and S N Raymond
Monthly Notices of the Royal Astronomical Society 488 (1) 645 (2019)
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