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The compositional diversity of rocky exoplanets around K-dwarf stars
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The effect of dynamic temperatures on pebble dynamics and planet formation
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JWST Reveals Excess Cool Water near the Snow Line in Compact Disks, Consistent with Pebble Drift
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Sublimation of refractory minerals in the gas envelopes of accreting rocky planets
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Formation of pebbles in (gravito-)viscous protoplanetary disks with various turbulent strengths
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Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury
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How dust fragmentation may be beneficial to planetary growth by pebble accretion
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Increased isolation mass for pebble accreting planetary cores in pressure maxima of protoplanetary discs
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Influences of protoplanet-induced three-dimensional gas flow on pebble accretion
A new and simple prescription for planet orbital migration and eccentricity damping by planet–disc interactions based on dynamical friction
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A giant exoplanet orbiting a very-low-mass star challenges planet formation models
J. C. Morales, A. J. Mustill, I. Ribas, M. B. Davies, A. Reiners, F. F. Bauer, D. Kossakowski, E. Herrero, E. Rodríguez, M. J. López-González, C. Rodríguez-López, V. J. S. Béjar, L. González-Cuesta, R. Luque, E. Pallé, M. Perger, D. Baroch, A. Johansen, H. Klahr, C. Mordasini, G. Anglada-Escudé, J. A. Caballero, M. Cortés-Contreras, S. Dreizler, M. Lafarga, et al. Science 365(6460) 1441 (2019) https://doi.org/10.1126/science.aax3198
Pebble accretion in self-gravitating protostellar discs