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astro-ph.EP2023
Rapid Dust Growth During Hydrodynamic Clumping Due to Streaming Instability
Ryosuke T. Tominaga, Hidekazu Tanaka
Streaming instability is considered to be one of the dominant processes to promote planetesimal formation by gravitational collapse of dust clumps. The development of streaming ins…
astro-ph.EP2023
Rapid Formation of Gas-giant Planets via Collisional Coagulation from Dust Grains to Planetary Cores. II. Dependence on Pebble Bulk Density and Disk Temperature
Hiroshi Kobayashi, Hidekazu Tanaka
Thanks to ``dust-to-planet'' simulations (DTPSs), which treat the collisional evolution directly from dust to giant-planet cores in a protoplanetary disk, we showed that giant-plan…