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Numerical simulations of the interaction between the stellar magnetic field and a planet
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Small and Close-in Planets are Uncommon Around A-type Stars
A fading radius valley towards M dwarfs, a persistent density valley across stellar types
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Dust-gas coupling in turbulence- and MHD wind-driven protoplanetary disks: Implications for rocky planet formation
The Inner Disk Rim of HD 163296: Linking Radiative Hydrostatic Models with Infrared Interferometry
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Study of type II migration under the framework of the disk instability model for giant planet formation
Gas, not dust: Migration of TESS/Gaia hot Jupiters possibly halted by the magnetospheres of protoplanetary disks
I. Mendigutía, J. Lillo-Box, M. Vioque, J. Maldonado, B. Montesinos, N. Huélamo and J. Wang Astronomy & Astrophysics 686 L1 (2024) https://doi.org/10.1051/0004-6361/202449368
The Impact-driven Atmospheric Loss of Super-Earths around Different Spectral Types of Host Stars
TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
J. Lillo-Box, D. Gandolfi, D. J. Armstrong, K. A. Collins, L. D. Nielsen, R. Luque, J. Korth, S. G. Sousa, S. N. Quinn, L. Acuña, S. B. Howell, G. Morello, C. Hellier, S. Giacalone, S. Hoyer, K. Stassun, E. Palle, A. Aguichine, O. Mousis, V. Adibekyan, T. Azevedo Silva, D. Barrado, M. Deleuil, J. D. Eastman, A. Fukui, et al. Astronomy & Astrophysics 669 A109 (2023) https://doi.org/10.1051/0004-6361/202243879
Formation of giant planets around intermediate-mass stars
The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
Erik A. Petigura, James G. Rogers, Howard Isaacson, James E. Owen, Adam L. Kraus, Joshua N. Winn, Mason G. MacDougall, Andrew W. Howard, Benjamin Fulton, Molly R. Kosiarek, Lauren M. Weiss, Aida Behmard and Sarah Blunt The Astronomical Journal 163(4) 179 (2022) https://doi.org/10.3847/1538-3881/ac51e3
Trapping (sub-)Neptunes similar to TOI-216b at the inner disk rim
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
Emerging population of gap-opening planets around type-A stars
The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at ≈2 au
Yunlin Zeng, Timothy D. Brandt, Gongjie Li, Trent J. Dupuy, Yiting Li, G. Mirek Brandt, Jay Farihi, Jonathan Horner, Robert A. Wittenmyer, R. Paul. Butler, Christopher G. Tinney, Bradley D. Carter, Duncan J. Wright, Hugh R. A. Jones and Simon J. O’Toole The Astronomical Journal 164(5) 188 (2022) https://doi.org/10.3847/1538-3881/ac8ff7
Probing the Inner Edge of Dead Zones in Protoplanetary Disks with ALMA and Next Generation Very Large Array
A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System*
Trifon Trifonov, Anna Wollbold, Martin Kürster, Jan Eberhardt, Stephan Stock, Thomas Henning, Sabine Reffert, R. Paul Butler, Steven S. Vogt, Ansgar Reiners, Man Hoi Lee, Bertram Bitsch, Mathias Zechmeister, Florian Rodler, Volker Perdelwitz, Lev Tal-Or, Jan Rybizki, Paul Heeren, Davide Gandolfi, Oscar Barragán, Olga Zakhozhay, Paula Sarkis, Marcelo Tala Pinto, Diana Kossakowski, Vera Wolthoff, et al. The Astronomical Journal 164(4) 156 (2022) https://doi.org/10.3847/1538-3881/ac7ce0
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
A “no-drift” runaway pile-up of pebbles in protoplanetary disks
Primordial dusty rings and episodic outbursts in protoplanetary discs
Kundan Kadam, Eduard Vorobyov and Shantanu Basu Monthly Notices of the Royal Astronomical Society 516(3) 4448 (2022) https://doi.org/10.1093/mnras/stac2455
Kepler-223 resonance holds information about turbulence during the gas-disk phase
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
The Nature and Origins of Sub‐Neptune Size Planets
The distribution of mutual inclinations arising from the stellar quadrupole moment
Kathleen Schultz, Christopher Spalding and Konstantin Batygin Monthly Notices of the Royal Astronomical Society 506(2) 2999 (2021) https://doi.org/10.1093/mnras/stab1899
The Effect of a Strong Pressure Bump in the Sun’s Natal Disk: Terrestrial Planet Formation via Planetesimal Accretion Rather than Pebble Accretion
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
MRI-active inner regions of protoplanetary discs. I. A detailed model of disc structure
Marija R Jankovic, James E Owen, Subhanjoy Mohanty and Jonathan C Tan Monthly Notices of the Royal Astronomical Society 504(1) 280 (2021) https://doi.org/10.1093/mnras/stab920
A bright inner disk and structures in the transition disk around the very low-mass star CIDA 1
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
The origins of nearly coplanar, non-resonant systems of close-in super-Earths
Leandro Esteves, André Izidoro, Sean N Raymond and Bertram Bitsch Monthly Notices of the Royal Astronomical Society 497(2) 2493 (2020) https://doi.org/10.1093/mnras/staa2112
Migration of gap-opening planets in 3D stellar-irradiated accretion disks
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
The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario