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N-body simulation of planetary formation through pebble accretion in a radially structured protoplanetary disk
Tenri Jinno, Takayuki R Saitoh, Yota Ishigaki and Junichiro Makino Publications of the Astronomical Society of Japan 75(5) 951 (2023) https://doi.org/10.1093/pasj/psad053
On the interaction of pebble accreting embryos with the gaseous disc: importance of thermal forces
Sonia Cornejo, Frédéric S Masset and F J Sánchez-Salcedo Monthly Notices of the Royal Astronomical Society 523(1) 936 (2023) https://doi.org/10.1093/mnras/stad1476
Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar system
Rapid formation of massive planetary cores in a pressure bump
Tommy Chi Ho Lau, Joanna Drążkowska, Sebastian M. Stammler, Tilman Birnstiel and Cornelis P. Dullemond Astronomy & Astrophysics 668 A170 (2022) https://doi.org/10.1051/0004-6361/202244864
Timing of Martian core formation from models of Hf–W evolution coupled with N-body simulations
Collision Chains among the Terrestrial Planets. III. Formation of the Moon
Erik Asphaug, Alexandre Emsenhuber, Saverio Cambioni, Travis S. J. Gabriel and Stephen R. Schwartz The Planetary Science Journal 2(5) 200 (2021) https://doi.org/10.3847/PSJ/ac19b2
How dust fragmentation may be beneficial to planetary growth by pebble accretion
A new and simple prescription for planet orbital migration and eccentricity damping by planet–disc interactions based on dynamical friction
Shigeru Ida, Takayuki Muto, Soko Matsumura and Ramon Brasser Monthly Notices of the Royal Astronomical Society 494(4) 5666 (2020) https://doi.org/10.1093/mnras/staa1073
Unified Simulations of Planetary Formation and Atmospheric Evolution: Effects of Pebble Accretion, Giant Impacts, and Stellar Irradiation on Super-Earth Formation
Promoted mass growth of multiple, distant giant planets through pebble accretion and planet–planet collision
Masahiro Ogihara, Beibei Liu and John Wimarsson Monthly Notices of the Royal Astronomical Society 496(3) 3314 (2020) https://doi.org/10.1093/mnras/staa1708
Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks
Orbital Motion of the Wide Planetary-mass Companion GSC 6214-210 b: No Evidence for Dynamical Scattering
Logan A. Pearce, Adam L. Kraus, Trent J. Dupuy, Michael J. Ireland, Aaron C. Rizzuto, Brendan P. Bowler, Eloise K. Birchall and Alexander L. Wallace The Astronomical Journal 157(2) 71 (2019) https://doi.org/10.3847/1538-3881/aafacb
Pebble-isolation mass: Scaling law and implications for the formation of super-Earths and gas giants