Articles citing this article

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Cited article:

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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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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)

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)

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

André Izidoro, Bertram Bitsch and Rajdeep Dasgupta
The Astrophysical Journal 915 (1) 62 (2021)

From dust to planets – I. Planetesimal and embryo formation

Gavin A L Coleman
Monthly Notices of the Royal Astronomical Society 506 (3) 3596 (2021)

Giant planet formation at the pressure maxima of protoplanetary disks

Octavio Miguel Guilera, Zsolt Sándor, María Paula Ronco, Julia Venturini and Marcelo Miguel Miller Bertolami
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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)

The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario

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Astronomy & Astrophysics 643 A66 (2020)

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)