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A Potential Site for Wide-orbit Giant Planet Formation in the IM Lup Disk
Arthur D. Bosman, Johan Appelgren, Edwin A. Bergin, Michiel Lambrechts and Anders Johansen The Astrophysical Journal Letters 944(2) L53 (2023) https://doi.org/10.3847/2041-8213/acb651
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
Planet population synthesis: the role of stellar encounters
Dust accumulation near the magnetospheric truncation of protoplanetary discs around T Tauri stars
Rixin Li(李日新), Yi-Xian Chen(陈逸贤) and Douglas N C Lin(林潮) Monthly Notices of the Royal Astronomical Society 510(4) 5246 (2022) https://doi.org/10.1093/mnras/stab3677
Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H α
The importance of thermal torques on the migration of planets growing by pebble accretion
Octavio M Guilera, Marcelo M Miller Bertolami, Frederic Masset, et al. Monthly Notices of the Royal Astronomical Society 507(3) 3638 (2021) https://doi.org/10.1093/mnras/stab2371
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
Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation
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
Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses