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Millimeter emission in photoevaporating disks is determined by early substructures
Matías Gárate, Til Birnstiel, Paola Pinilla, Sean M. Andrews, Raphael Franz, Sebastian Markus Stammler, Giovanni Picogna, Barbara Ercolano, Anna Miotello and Nicolás T. Kurtovic Astronomy & Astrophysics 679 A15 (2023) https://doi.org/10.1051/0004-6361/202244436
In situ enrichment in heavy elements of hot Jupiters
The role of density perturbation on planet formation by pebble accretion
G Andama, N Ndugu, S K Anguma and E Jurua Monthly Notices of the Royal Astronomical Society 512(4) 5278 (2022) https://doi.org/10.1093/mnras/stac772
Protostellar collapse simulations in spherical geometry with dust coagulation and fragmentation
Ugo Lebreuilly, Valentin Vallucci-Goy, Vincent Guillet, Maxime Lombart and Pierre Marchand Monthly Notices of the Royal Astronomical Society 518(3) 3326 (2022) https://doi.org/10.1093/mnras/stac3220
Presolar grain dynamics: Creating nucleosynthetic variations through a combination of drag and viscous evolution
Mark A Hutchison, Jean-David Bodénan, Lucio Mayer and Maria Schönbächler Monthly Notices of the Royal Astronomical Society 512(4) 5874 (2022) https://doi.org/10.1093/mnras/stac765
Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. I. First Numerical Study of Accelerated Dust Growth and Dust Concentration at Outer Radii
ALMA constraints on assembly of core accretion planets
Sergei Nayakshin, Vardan Elbakyan and Giovanni Rosotti Monthly Notices of the Royal Astronomical Society 512(4) 6038 (2022) https://doi.org/10.1093/mnras/stac833
The impact of dynamic pressure bumps on the observational properties of protoplanetary disks
On dust evolution in planet-forming discs in binary systems – I. Theoretical and numerical modelling: radial drift is faster in binary discs
Francesco Zagaria, Giovanni P Rosotti and Giuseppe Lodato Monthly Notices of the Royal Astronomical Society 504(2) 2235 (2021) https://doi.org/10.1093/mnras/stab985
Spiral structures in gravito-turbulent gaseous disks
MRI-active inner regions of protoplanetary discs – II. Dependence on dust, disc, and stellar parameters
Marija R Jankovic, Subhanjoy Mohanty, James E Owen and Jonathan C Tan Monthly Notices of the Royal Astronomical Society 509(4) 5974 (2021) https://doi.org/10.1093/mnras/stab3370
Large gaps and high accretion rates in photoevaporative transition disks with a dead zone
Dust growth, fragmentation, and self-induced dust traps in phantom
Arnaud Vericel, Jean-François Gonzalez, Daniel J Price, Guillaume Laibe and Christophe Pinte Monthly Notices of the Royal Astronomical Society 507(2) 2318 (2021) https://doi.org/10.1093/mnras/stab2263
Dust entrainment in photoevaporative winds: The impact of X-rays
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
Gas accretion damped by dust back-reaction at the snow line
The time evolution of dusty protoplanetary disc radii: observed and physical radii differ
Cathie Clarke, Giuseppe Lodato, Leonardo Testi, et al. Monthly Notices of the Royal Astronomical Society 486(4) 4829 (2019) https://doi.org/10.1093/mnras/stz1190
Tracking Dust Grains during Transport and Growth in Protoplanetary Disks
Physics of planet trapping with applications to HL Tau
Alexander J Cridland, Ralph E Pudritz and Matthew Alessi Monthly Notices of the Royal Astronomical Society 484(1) 345 (2019) https://doi.org/10.1093/mnras/stz008
Growth and Settling of Dust Particles in Protoplanetary Nebulae: Implications for Opacity, Thermal Profile, and Gravitational Instability
Debanjan Sengupta, Sarah E. Dodson-Robinson, Yasuhiro Hasegawa and Neal J. Turner The Astrophysical Journal 874(1) 26 (2019) https://doi.org/10.3847/1538-4357/aafc36
Characterizing the Variable Dust Permeability of Planet-induced Gaps
Philipp Weber, Pablo Benítez-Llambay, Oliver Gressel, Leonardo Krapp and Martin E. Pessah The Astrophysical Journal 854(2) 153 (2018) https://doi.org/10.3847/1538-4357/aaab63
Collisional Growth of Icy Dust Aggregates in the Disk Formation Stage: Difficulties for Planetesimal Formation via Direct Collisional Growth outside the Snowline
The structure of young embedded protostellar discs
Benjamin A. MacFarlane and Dimitris Stamatellos Monthly Notices of the Royal Astronomical Society 472(4) 3775 (2017) https://doi.org/10.1093/mnras/stx1973
The Effects of Protostellar Disk Turbulence on CO Emission Lines: A Comparison Study of Disks with Constant CO Abundance versus Chemically Evolving Disks
Mo Yu, Neal J. Evans, Sarah E. Dodson-Robinson, Karen Willacy and Neal J. Turner The Astrophysical Journal 850(2) 169 (2017) https://doi.org/10.3847/1538-4357/aa9217
Apparent Disk-mass Reduction and Planetisimal Formation in GravitationallyUnstable Disks in Class 0/I Young Stellar Objects
X-ray photoevaporation’s limited success in the formation of planetesimals by the streaming instability
Barbara Ercolano, Jeff Jennings, Giovanni Rosotti and Tilman Birnstiel Monthly Notices of the Royal Astronomical Society 472(4) 4117 (2017) https://doi.org/10.1093/mnras/stx2294
Disk Masses around Solar-mass Stars are Underestimated by CO Observations
Mo Yu, Neal J. Evans II, Sarah E. Dodson-Robinson, Karen Willacy and Neal J. Turner The Astrophysical Journal 841(1) 39 (2017) https://doi.org/10.3847/1538-4357/aa6e4c
Effects of Grain Growth on Molecular Abundances in Young Stellar Objects
Radial drift of dust in protoplanetary discs: the evolution of ice lines and dead zones
A. J. Cridland, Ralph E. Pudritz and T. Birnstiel Monthly Notices of the Royal Astronomical Society 465(4) 3865 (2017) https://doi.org/10.1093/mnras/stw2946
GLOBAL MODELING OF NEBULAE WITH PARTICLE GROWTH, DRIFT, AND EVAPORATION FRONTS. I. METHODOLOGY AND TYPICAL RESULTS
Growing dust grains in protoplanetary discs – I. Radial drift with toy growth models
Guillaume Laibe, Jean-François Gonzalez and Sarah T. Maddison Monthly Notices of the Royal Astronomical Society 437(4) 3025 (2014) https://doi.org/10.1093/mnras/stt1927
THE EVOLUTION OF ACCRETION IN YOUNG STELLAR OBJECTS: STRONG ACCRETORS AT 3-10 Myr