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Gravitoviscous protoplanetary disks with a dust component

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Transport, Destruction, and Growth of Pebbles in the Gas Envelope of a Protoplanet

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

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

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Formation of planetary systems by pebble accretion and migration

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Astronomy & Astrophysics 627 A83 (2019)
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Are the observed gaps in protoplanetary discs caused by growing planets?

N Ndugu, B Bitsch and E Jurua
Monthly Notices of the Royal Astronomical Society 488 (3) 3625 (2019)
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A giant exoplanet orbiting a very-low-mass star challenges planet formation models

J. C. Morales, A. J. Mustill, I. Ribas, M. B. Davies, A. Reiners, F. F. Bauer, D. Kossakowski, E. Herrero, E. Rodríguez, M. J. López-González, C. Rodríguez-López, V. J. S. Béjar, L. González-Cuesta, R. Luque, E. Pallé, M. Perger, D. Baroch, A. Johansen, H. Klahr, C. Mordasini, G. Anglada-Escudé, J. A. Caballero, M. Cortés-Contreras, S. Dreizler, M. Lafarga, et al.
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Formation of planetary systems by pebble accretion and migration: growth of gas giants

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Planet-forming material in a protoplanetary disc: the interplay between chemical evolution and pebble drift

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The Galilean Satellites Formed Slowly from Pebbles

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Super-Earth masses sculpted by pebble isolation around stars of different masses

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Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks

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The newborn planet population emerging from ring-like structures in discs

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