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Predicting the Dominant Formation Mechanism of Multiplanetary Systems
Cheyanne Shariat, Yasuhiro Hasegawa, Bradley M. S. Hansen, Tze Yeung Mathew Yu and Renyu Hu The Astrophysical Journal Letters 964(1) L13 (2024) https://doi.org/10.3847/2041-8213/ad2c8d
Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes
A radius valley between migrated steam worlds and evaporated rocky cores
Remo Burn, Christoph Mordasini, Lokesh Mishra, Jonas Haldemann, Julia Venturini, Alexandre Emsenhuber and Thomas Henning Nature Astronomy 8(4) 463 (2024) https://doi.org/10.1038/s41550-023-02183-7
The Prevalence of Resonance Among Young, Close-in Planets
Fei Dai, Max Goldberg, Konstantin Batygin, Jennifer van Saders, Eugene Chiang, Nick Choksi, Rixin Li, Erik A. Petigura, Gregory J. Gilbert, Sarah C. Millholland, Yuan-Zhe Dai, Luke Bouma, Lauren M. Weiss and Joshua N. Winn The Astronomical Journal 168(6) 239 (2024) https://doi.org/10.3847/1538-3881/ad83a6
The stability of unevenly spaced planetary systems
The Exoplanet Radius Valley from Gas-driven Planet Migration and Breaking of Resonant Chains
André Izidoro, Hilke E. Schlichting, Andrea Isella, Rajdeep Dasgupta, Christian Zimmermann and Bertram Bitsch The Astrophysical Journal Letters 939(2) L19 (2022) https://doi.org/10.3847/2041-8213/ac990d
TRAPPIST-1: Dynamical analysis of the transit-timing variations and origin of the resonant chain
Sean N. Raymond and Alessandro Morbidelli Astrophysics and Space Science Library, Demographics of Exoplanetary Systems 466 3 (2022) https://doi.org/10.1007/978-3-030-88124-5_1
Habitable Planet Formation around Low-mass Stars: Rapid Accretion, Rapid Debris Removal, and the Essential Contribution of External Giants
K. Biazzo, V. Bozza, L. Mancini and A. Sozzetti Astrophysics and Space Science Library, Demographics of Exoplanetary Systems 466 143 (2022) https://doi.org/10.1007/978-3-030-88124-5_3
The New Generation Planetary Population Synthesis (NGPPS)
Early Initiation of Inner Solar System Formation at the Dead-zone Inner Edge
Takahiro Ueda, Masahiro Ogihara, Eiichiro Kokubo and Satoshi Okuzumi The Astrophysical Journal Letters 921(1) L5 (2021) https://doi.org/10.3847/2041-8213/ac2f3b
A pebble accretion model for the formation of the terrestrial planets in the Solar System
Anders Johansen, Thomas Ronnet, Martin Bizzarro, Martin Schiller, Michiel Lambrechts, Åke Nordlund and Helmut Lammer Science Advances 7(8) (2021) https://doi.org/10.1126/sciadv.abc0444
The ‘breaking the chains’ migration model for super-Earth formation: the effect of collisional fragmentation
Leandro Esteves, André Izidoro, Bertram Bitsch, et al. Monthly Notices of the Royal Astronomical Society 509(2) 2856 (2021) https://doi.org/10.1093/mnras/stab3203
Departure from the Exact Location of Mean Motion Resonances Induced by the Gas Disk in Systems Observed by Kepler
Molecules with ALMA at Planet-forming Scales (MAPS). XVI. Characterizing the Impact of the Molecular Wind on the Evolution of the HD 163296 System
Alice S. Booth, Benoît Tabone, John D. Ilee, Catherine Walsh, Yuri Aikawa, Sean M. Andrews, Jaehan Bae, Edwin A. Bergin, Jennifer B. Bergner, Arthur D. Bosman, Jenny K. Calahan, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Viviana V. Guzmán, Jane Huang, Charles J. Law, Romane Le Gal, Feng Long, Ryan A. Loomis, François Ménard, Hideko Nomura, Karin I. Öberg, Chunhua Qi, Kamber R. Schwarz, et al. The Astrophysical Journal Supplement Series 257(1) 16 (2021) https://doi.org/10.3847/1538-4365/ac1ad4
A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)
Giant planet formation at the pressure maxima of protoplanetary disks
Octavio Miguel Guilera, Zsolt Sándor, María Paula Ronco, Julia Venturini and Marcelo Miguel Miller Bertolami Astronomy & Astrophysics 642 A140 (2020) https://doi.org/10.1051/0004-6361/202038458
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
Formation of planetary populations − II. Effects of initial disc size and radial dust drift
Matthew Alessi, Ralph E Pudritz and Alex J Cridland Monthly Notices of the Royal Astronomical Society 493(1) 1013 (2020) https://doi.org/10.1093/mnras/staa308
Do the TRAPPIST-1 Planets Have Hydrogen-rich Atmospheres?
Julia Venturini, Octavio M. Guilera, Jonas Haldemann, María P. Ronco and Christoph Mordasini Astronomy & Astrophysics 643 L1 (2020) https://doi.org/10.1051/0004-6361/202039141
Ejection of close-in super-Earths around low-mass stars in the giant impact stage
Unified Simulations of Planetary Formation and Atmospheric Evolution. II. Rapid Disk Clearing by Photoevaporation Yields Low-mass Super-Earth Atmospheres
The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines
Ilaria Pascucci, Andrea Banzatti, Uma Gorti, Min Fang, Klaus Pontoppidan, Richard Alexander, Giulia Ballabio, Suzan Edwards, Colette Salyk, Germano Sacco, Ettore Flaccomio, Geoffrey A. Blake, Andres Carmona, Cassandra Hall, Inga Kamp, Hans Ulrich Käufl, Gwendolyn Meeus, Michael Meyer, Tyler Pauly, Simon Steendam and Michael Sterzik The Astrophysical Journal 903(2) 78 (2020) https://doi.org/10.3847/1538-4357/abba3c
Unified Simulations of Planetary Formation and Atmospheric Evolution: Effects of Pebble Accretion, Giant Impacts, and Stellar Irradiation on Super-Earth Formation
Time-dependent evolution of the protoplanetary discs with magnetic winds
Mohsen Shadmehri and Sayyedeh Masoumeh Ghoreyshi Monthly Notices of the Royal Astronomical Society 488(4) 4623 (2019) https://doi.org/10.1093/mnras/stz2025
Close-in Super-Earths: The first and the last stages of planet formation in an MRI-accreting disc
Marija R Jankovic, James E Owen and Subhanjoy Mohanty Monthly Notices of the Royal Astronomical Society 484(2) 2296 (2019) https://doi.org/10.1093/mnras/stz004
Inner rocky super-Earth formation: distinguishing the formation pathways in viscously heated and passive discs