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Material transport in protoplanetary discs with massive embedded planets
Hannah J Petrovic, Richard A Booth and Cathie J Clarke Monthly Notices of the Royal Astronomical Society 534(3) 2412 (2024) https://doi.org/10.1093/mnras/stae2229
How external photoevaporation changes the chemical composition of the inner disc
Using the Ca ii Lines in T Tauri Stars to Infer the Abundance of Refractory Elements in the Innermost Disk Region
Marbely Micolta, Nuria Calvet, Thanawuth Thanathibodee, Gladis Magris C., Carlo F. Manara, Laura Venuti, Juan Manuel Alcalá and Gregory J. Herczeg The Astrophysical Journal 976(2) 251 (2024) https://doi.org/10.3847/1538-4357/ad8884
Water Enrichment from Pebble Drift in Disks with Gap-forming Planets
An impact-free mechanism to deliver water to terrestrial planets and exoplanets
Quentin Kral, Paul Huet, Camille Bergez-Casalou, Philippe Thébault, Sébastien Charnoz and Sonia Fornasier Astronomy & Astrophysics 692 A70 (2024) https://doi.org/10.1051/0004-6361/202451263
Atmospheric recycling of volatiles by pebble-accreting planets
Yu Wang, Chris W Ormel, Pinghui Huang and Rolf Kuiper Monthly Notices of the Royal Astronomical Society 523(4) 6186 (2023) https://doi.org/10.1093/mnras/stad1753
Giants are bullies: How their growth influences systems of inner sub-Neptunes and super-Earths
Interpreting the Atmospheric Composition of Exoplanets: Sensitivity to Planet Formation Assumptions
Paul Mollière, Tamara Molyarova, Bertram Bitsch, Thomas Henning, Aaron Schneider, Laura Kreidberg, Christian Eistrup, Remo Burn, Evert Nasedkin, Dmitry Semenov, Christoph Mordasini, Martin Schlecker, Kamber R. Schwarz, Sylvestre Lacour, Mathias Nowak and Matthäus Schulik The Astrophysical Journal 934(1) 74 (2022) https://doi.org/10.3847/1538-4357/ac6a56
Trapping (sub-)Neptunes similar to TOI-216b at the inner disk rim
Which planets trigger longer lived vortices: low-mass or high-mass?
Michael Hammer, Min-Kai Lin, Kaitlin M Kratter and Paola Pinilla Monthly Notices of the Royal Astronomical Society 504(3) 3963 (2021) https://doi.org/10.1093/mnras/stab1079
Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line
Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario
N Ndugu, B Bitsch, A Morbidelli, A Crida and E Jurua Monthly Notices of the Royal Astronomical Society 501(2) 2017 (2021) https://doi.org/10.1093/mnras/staa3629