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Gap opening in protoplanetary discs: gas dynamics from global axisymmetric non-ideal MHD simulations with consistent thermochemistry

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Spin of protoplanets generated by pebble accretion: Influences of protoplanet-induced gas flow

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Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?

Linn E J Eriksson, Marit A S Mol Lous, Sho Shibata and Ravit Helled
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Planet formation via pebble accretion in externally photoevaporating discs

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Composition constraints of the TRAPPIST-1 planets from their formation

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Disc population synthesis: Decrease in the solid mass reservoir through pebble drift

J. Appelgren, M. Lambrechts and N. van der Marel
Astronomy & Astrophysics 673 A139 (2023)
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How the planetary eccentricity influences the pebble isolation mass

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Rapid formation of massive planetary cores in a pressure bump

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Recycling of the first atmospheres of embedded planets: Dependence on core mass and optical depth

T. W. Moldenhauer, R. Kuiper, W. Kley and C. W. Ormel
Astronomy & Astrophysics 661 A142 (2022)
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A strong H− opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b

B. Jacobs, J.-M. Désert, L. Pino, et al.
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