Showing 1–20 of 28 results
/ Date/ Name
Apr 13, 2018Identifying inflated super-Earths and photo-evaporated coresMar 5, 2019Formation of short-period planets by disk migrationAug 18, 2021Resilience of Planetesimal Formation in Weakly-Reinforced Pressure BumpsApr 7, 2016How to form asteroids from mm-sized grainsApr 29, 2022The Streaming Instability Cannot Form Planetesimals from mm-size Grains in Pressure BumpsJan 21, 2015How to form planetesimals from mm-sized chondrules and chondrule aggregatesMay 4, 2016Survival of habitable planets in unstable planetary systemsMar 25, 2017Toward an initial mass function for giant planetsMar 5, 2025Positive Feedback: How a Synergy Between the Streaming Instability and Dust Coagulation Forms PlanetesimalsApr 8, 2025Positive Feedback II: How Dust Coagulation inside Vortices Can Form Planetesimals at Low MetallicityMar 4, 2026A Comparative Study of the Streaming Instability: Unstratified Models with Marginally Coupled GrainsMar 1, 2021Rapid Formation of Super-Earths Around Low-Mass StarsMar 6, 2019Planet-planet scattering as the source of the highest eccentricity exoplanetsApr 10, 2024Magnetically Driven Turbulence in the Inner Regions of Protoplanetary DisksJan 9, 2024A solution for the density dichotomy problem of Kuiper Belt objects with multi-species streaming instability and pebble accretionMar 14, 2025Planets and planetesimals at cosmic dawn: Vortices as planetary nurseriesAug 4, 2020Protoplanetary Disk Rings as Sites for Planetesimal FormationMar 23, 2017Planetesimal formation by the streaming instability in a photoevaporating diskApr 17, 2025Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to InfallFeb 10, 2022Migration traps as the root cause of the Kepler dichotomy