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Cited article:

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Thermal torque effects on the migration of growing low-mass planets

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Super-Earths in the TW Hya disc

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The formation of Jupiter’s diluted core by a giant impact

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Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

Joanna Dra̧żkowska, Shengtai Li, Til Birnstiel, Sebastian M. Stammler and Hui Li
The Astrophysical Journal 885 (1) 91 (2019)
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The Galilean Satellites Formed Slowly from Pebbles

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Vortex instabilities triggered by low-mass planets in pebble-rich, inviscid protoplanetary discs

A Pierens, M-K Lin and S N Raymond
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Are the observed gaps in protoplanetary discs caused by growing planets?

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Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks

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Super-Earth masses sculpted by pebble isolation around stars of different masses

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Migrating super-Earths in low-viscosity discs: unveiling the roles of feedback, vortices, and laminar accretion flows

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Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion, and disc evolution

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Astronomy & Astrophysics 624 A109 (2019)
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Is the ring inside or outside the planet?: the effect of planet migration on dust rings

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Metallicity effect and planet mass function in pebble-based planet formation models

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The Origin of the Heavy-element Content Trend in Giant Planets via Core Accretion

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