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Dust Recycling and Icy Volatile Enhancement (DRIVE): A Novel Method of Volatile Enrichment in Cold Giant Planets
Eric R. Van Clepper, Felipe Alarcón, Edwin Bergin and Fred J. Ciesla The Astrophysical Journal Letters 994(2) L44 (2025) https://doi.org/10.3847/2041-8213/ae1d81
Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation
Tommy Chi Ho 智昊 Lau 劉, Til Birnstiel, Sebastian M. Stammler and Joanna Drążkowska The Astrophysical Journal 994(1) 74 (2025) https://doi.org/10.3847/1538-4357/ae0c17
The New Generation Planetary Population Synthesis (NGPPS)
Alexandre Emsenhuber, Christoph Mordasini, Michel Mayor, Maxime Marmier, Stéphane Udry, Remo Burn, Martin Schlecker, Lokesh Mishra, Yann Alibert, Willy Benz and Erik Asphaug Astronomy & Astrophysics 701 A64 (2025) https://doi.org/10.1051/0004-6361/202452485
Accretion of Uranus and Neptune: Confronting different giant impact scenarios
Planetesimal formation in a pressure bump induced by infall
Haichen Zhao, Tommy Chi Ho Lau, Tilman Birnstiel, Sebastian M. Stammler and Joanna Dra̧żkowska Astronomy & Astrophysics 694 A205 (2025) https://doi.org/10.1051/0004-6361/202452941
A primordial radius valley as a consequence of planet formation
Refractory carbon depletion by photolysis through dust collisions and vertical mixing
Vignesh Vaikundaraman, Joanna Drążkowska, Fabian Binkert, Til Birnstiel and Anna Miotello Astronomy & Astrophysics 696 A215 (2025) https://doi.org/10.1051/0004-6361/202553850
Can close-in exoplanets form by pebble accretion?
Jayashree Narayan, Joanna Drążkowska and Vignesh Vaikundaraman Monthly Notices of the Royal Astronomical Society 540(1) 165 (2025) https://doi.org/10.1093/mnras/staf734
Spirals, rings, and vortices shaped by shadows in protoplanetary discs: from radiative hydrodynamical simulations to observable signatures
Multi-frequency analysis of the ALMA and VLA high resolution continuum observations of the substructured disc around CI Tau
Francesco Zagaria, Stefano Facchini, Pietro Curone, Jonathan P. Williams, Cathie J. Clarke, Álvaro Ribas, Marco Tazzari, Enrique Macías, Richard A. Booth, Giovanni P. Rosotti and Leonardo Testi Astronomy & Astrophysics 702 A56 (2025) https://doi.org/10.1051/0004-6361/202452986
Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall
Daniel Carrera, Abigail Davenport, Jacob B. Simon, Hans Baehr, Til Birnstiel, Cassandra Hall, David Rea and Sebastian Markus Stammler The Astrophysical Journal 990(1) 39 (2025) https://doi.org/10.3847/1538-4357/adef46
Cosmic Cascades: How Disk Substructure Regulates the Flow of Water to Inner Planetary Systems
Sebastiaan Krijt, Andrea Banzatti, Ke Zhang, Paola Pinilla, Till Kaeufer, Edwin A. Bergin, Colette Salyk, Klaus Pontoppidan, Geoffrey A. Blake, Feng Long, Jane Huang, María José Colmenares, Joe Williams, Adrien Houge, Mayank Narang, Miguel Vioque, Michiel Lambrechts, L. Ilsedore Cleeves and Karin Öberg The Astrophysical Journal Letters 990(2) L72 (2025) https://doi.org/10.3847/2041-8213/adfbe3
Ralph E. Pudritz, Alex J. Cridland, Julie Inglis and Matthew Alessi 1 (2025) https://doi.org/10.1007/978-3-319-30648-3_144-2
Giant planet formation via pebble accretion across different stellar masses
Yves Marrocchi, Rhian H. Jones, Sara S. Russell, Dominik C. Hezel, Jens Barosch and Aleksandra Kuznetsova Space Science Reviews 220(6) (2024) https://doi.org/10.1007/s11214-024-01102-0
Dust rings trap protoplanets on eccentric orbits and get consumed by them
David A Velasco-Romero, Frédéric S Masset, Alessandro Morbidelli, Pablo Benítez-Llambay, Leonardo Krapp and Elena Lega Monthly Notices of the Royal Astronomical Society 533(1) 807 (2024) https://doi.org/10.1093/mnras/stae1835
Probing Dust and Gas Properties Using Ringed Disks
Sandwiched planet formation: restricting the mass of a middle planet
Matthew Pritchard, Farzana Meru, Sahl Rowther, David Armstrong and Kaleb Randall Monthly Notices of the Royal Astronomical Society 528(4) 6538 (2024) https://doi.org/10.1093/mnras/stad3163
Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?
Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS
J. A. Egger, H. P. Osborn, D. Kubyshkina, C. Mordasini, Y. Alibert, M. N. Günther, M. Lendl, A. Brandeker, A. Heitzmann, A. Leleu, M. Damasso, A. Bonfanti, T. G. Wilson, S. G. Sousa, J. Haldemann, L. Delrez, M. J. Hooton, T. Zingales, R. Luque, R. Alonso, J. Asquier, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, et al. Astronomy & Astrophysics 688 A223 (2024) https://doi.org/10.1051/0004-6361/202450472
Planet Formation—Observational Constraints, Physical Processes, and Compositional Patterns
Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?
Linn E J Eriksson, Marit A S Mol Lous, Sho Shibata and Ravit Helled Monthly Notices of the Royal Astronomical Society 526(4) 4860 (2023) https://doi.org/10.1093/mnras/stad3007
Planetesimal Growth in Evolving Protoplanetary Disks: Constraints from the Pebble Supply
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
Filling in the gaps: can gravitationally unstable discs form the seeds of gas giant planets?