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Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation

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Planetary core formation via multispecies pebble accretion

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Tidal pull of the Earth strips the proto-Moon of its volatiles

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The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks

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Pebble drift and planetesimal formation in protoplanetary discs with embedded planets

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Requirements for Gravitational Collapse in Planetesimal Formation—The Impact of Scales Set by Kelvin–Helmholtz and Nonlinear Streaming Instability

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The evolution of a circumplanetary disc with a dead zone

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Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses

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Giant planet formation at the pressure maxima of protoplanetary disks

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