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Circumplanetary Disks are Rare Around Planets at Large Orbital Radii: A Parameter Survey of Flow Morphology Around Giant Planets

We investigate how the formation and structure of circumplanetary disks (CPDs) vary with planet mass and protoplanetary disk aspect ratio. Using static mesh refinement and a near-isothermal equation of state, we perform a small parameter survey of hydrodynamic simulations with parameters appropriate...

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Principais autores: Sabina Sagynbayeva, Rixin Li, Aleksandra Kuznetsova, Zhaohuan Zhu, Yan-Fei Jiang, Philip J. Armitage
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2025-01-01
coleção:The Astrophysical Journal
Assuntos:
Protoplanetary disks
Planet formation
Exoplanet formation
Hydrodynamical simulations
Natural satellite formation
Acesso em linha:https://doi.org/10.3847/1538-4357/add934
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