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Turbulence in Particle-laden Midplane Layers of Planet-forming Disks

We examine the settled particle layers of planet-forming disks in which the streaming instability (SI) is thought to be either weak or inactive. A suite of low-to-moderate-resolution 3D simulations in a 0.2 H -sized box, where H is the pressure scale height, are performed using PENCIL for two Stokes...

Ausführliche Beschreibung

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Bibliografische Detailangaben
Hauptverfasser: Debanjan Sengupta, Orkan M. Umurhan
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2023-01-01
Schriftenreihe:The Astrophysical Journal
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Online-Zugang:https://doi.org/10.3847/1538-4357/ac9411
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