Astrophysics of Planet Formation
Author:
Publisher
Cambridge University Press
Reference376 articles.
1. Diagrammatic theory of transition of pendulum like systems
2. Concentrating small particles in protoplanetary disks through the streaming instability
3. Planet Migration and Binary Companions: The Case of HD 80606b
4. HOT STARS WITH HOT JUPITERS HAVE HIGH OBLIQUITIES
5. The distribution of mass in the planetary system and solar nebula
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1. Dust-gas coupling in turbulence- and MHD wind-driven protoplanetary disks: Implications for rocky planet formation;Icarus;2024-07
2. Three-temperature radiation hydrodynamics with PLUTO: Thermal and kinematic signatures of accreting protoplanets;Astronomy & Astrophysics;2024-07
3. Host-star Properties of Hot, Warm, and Cold Jupiters in the Solar Neighborhood from Gaia Data Release 3: Clues to Formation Pathways;The Astronomical Journal;2024-06-05
4. Thermal Structure Determines Kinematics: Vertical Shear Instability in Stellar Irradiated Protoplanetary Disks;The Astrophysical Journal;2024-06-01
5. DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs;Astronomy & Astrophysics;2024-05
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