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Cited article:

Planet Formation—Observational Constraints, Physical Processes, and Compositional Patterns

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Constraints on the formation history and composition of Kepler planets from their distribution of orbital period ratios

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Astronomy & Astrophysics 687 A25 (2024)
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The interplay between pebble and planetesimal accretion in population synthesis models and its role in giant planet formation

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From Pebbles and Planetesimals to Planets and Dust: The Protoplanetary Disk–Debris Disk Connection

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The Astrophysical Journal 925 (1) 45 (2022)
https://doi.org/10.3847/1538-4357/ac37b6

SimAb: A simple, fast, and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants

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Testing the Jeans, Toomre, and Bonnor–Ebert Concepts for Planetesimal Formation: 3D Streaming-instability Simulations of Diffusion-regulated Formation of Planetesimals

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The Astrophysical Journal 911 (1) 9 (2021)
https://doi.org/10.3847/1538-4357/abca9b

Second-generation dust in planetary systems: the case of HD 163296

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Monthly Notices of the Royal Astronomical Society 509 (3) 3181 (2021)
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Kepler-223 resonance holds information about turbulence during the gas-disk phase

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The Effect of a Strong Pressure Bump in the Sun’s Natal Disk: Terrestrial Planet Formation via Planetesimal Accretion Rather than Pebble Accretion

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The Astrophysical Journal 915 (1) 62 (2021)
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From dust to planets – I. Planetesimal and embryo formation

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Giant planet formation at the pressure maxima of protoplanetary disks

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Planet formation and disc mass dependence in a pebble-driven scenario for low-mass stars

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Monthly Notices of the Royal Astronomical Society 499 (3) 3510 (2020)
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The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario

Bertram Bitsch, Trifon Trifonov and Andre Izidoro
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Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses

Julia Venturini, Octavio Miguel Guilera, María Paula Ronco and Christoph Mordasini
Astronomy & Astrophysics 644 A174 (2020)
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