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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Bibliografische gegevens

Hoofdauteurs:	Sabina Sagynbayeva, Rixin Li, Aleksandra Kuznetsova, Zhaohuan Zhu, Yan-Fei Jiang, Philip J. Armitage
Formaat:	Artigo
Taal:	Inglês
Gepubliceerd in:	IOP Publishing 2025-01-01
Reeks:	The Astrophysical Journal
Onderwerpen:	Protoplanetary disks Planet formation Exoplanet formation Hydrodynamical simulations Natural satellite formation
Online toegang:	https://doi.org/10.3847/1538-4357/add934
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