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From streaming instability to the onset of pebble accretion
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Lauren Doyle, David J Armstrong, Lorena Acuña, Ares Osborn, Sérgio A G Sousa, Amadeo Castro-González, Vincent Bourrier, Douglas Alves, David Barrado, Susana C C Barros, Daniel Bayliss, Kaiming Cui, Olivier Demangeon, Rodrigo F Díaz, Xavier Dumusque, Fintan Eeles-Nolle, Samuel Gill, Alejandro Hacker, James S Jenkins, Marcelo Aron Fetzner Keniger, Marina Lafarga, Jorge Lillo-Box, Isobel Lockley, Louise D Nielsen, Léna Parc, et al. Monthly Notices of the Royal Astronomical Society 539(4) 3138 (2025) https://doi.org/10.1093/mnras/staf670
Building Earth with pebbles made of chondritic components
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Global N-body simulations of circumbinary planet formation around Kepler-16 and -34 analogues I: Exploring the pebble accretion scenario
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Accretion of ice giant planets from massive protoplanets whose migration is blocked by Jupiter and Saturn
G Benedetti-Rossi, R Ribeiro, O C Winter, H S Gaspar and E Vieira-Neto Monthly Notices of the Royal Astronomical Society 526(3) 4435 (2023) https://doi.org/10.1093/mnras/stad3017
N-body simulation of planetary formation through pebble accretion in a radially structured protoplanetary disk
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Migration processes in the Solar System and their role in the evolution of the Earth and planets
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Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system
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Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury