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Cited article:

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A tornado-based laboratory model for Keplerian flows

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The CO-fuelled Time Machine: tracing birth conditions and Terrestrial Planet Formation Outcomes in HD 163296 through Pebble Drift-induced CO Enhancements

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From small dust to micron-sized aggregates: The influence of structure and composition on the dust optical properties

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The growth of super-large pre-planetary pebbles to an impact erosion limit

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Smuggling unnoticed: towards a 2D view of water and dust delivery to the inner regions of protoplanetary discs

Adrien Houge, Sebastiaan Krijt, Andrea Banzatti, Geoffrey A Blake, Paola Pinilla, Klaus M Pontoppidan, Leon Trapman, Joe Williams and Ke Zhang
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Three-dimensional Transport of Solids in a Protoplanetary Disk Containing a Growing Giant Planet

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The Astrophysical Journal 980 (2) 201 (2025)
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Water in Protoplanetary Disks with JWST-MIRI: Spectral Excitation Atlas and Radial Distribution from Temperature Diagnostic Diagrams and Doppler Mapping

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From streaming instability to the onset of pebble accretion

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Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks

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Long-term evolution of the temperature structure in magnetized protoplanetary disks and its implication for the dichotomy of planetary composition

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Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux

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Forming giant planets around late-M dwarfs: Pebble accretion and planet–planet collision

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The Early Solar System and Its Meteoritical Witnesses

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A fading radius valley towards M dwarfs, a persistent density valley across stellar types

J. Venturini, M. P. Ronco, O. M. Guilera, J. Haldemann, C. Mordasini and M. Miller Bertolami
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Planetesimal formation via the streaming instability with multiple grain sizes

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Planetesimal Growth in Evolving Protoplanetary Disks: Constraints from the Pebble Supply

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The Astrophysical Journal 948 (2) 98 (2023)
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An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion

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The Astrophysical Journal 946 (2) 60 (2023)
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Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?

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Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets

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The Astrophysical Journal 953 (1) 97 (2023)
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Rapid formation of massive planetary cores in a pressure bump

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Tensile strength and surface energy of CO2 ice in the context of planet formation

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The growth and migration of massive planets under the influence of external photoevaporation

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Razor-thin dust layers in protoplanetary disks: Limits on the vertical shear instability

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Growth after the streaming instability: The radial distance dependence of the planetary growth

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Astronomy & Astrophysics 664 A86 (2022)
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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

Efficient planet formation by pebble accretion in ALMA rings

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Planet population synthesis: the role of stellar encounters

N Ndugu, O P Abedigamba and G Andama
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https://doi.org/10.1093/mnras/stac569

Single-dish 1-cm-band radio photometry of protoplanetary discs: few centimetre-sized dust grains?

Jane S Greaves and Brian Mason
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Resilience of Planetesimal Formation in Weakly Reinforced Pressure Bumps

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Formation of dust rings and gaps in non-ideal MHD discs through meridional gas flows

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The formation of wide exoKuiper belts from migrating dust traps

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