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Large Fluctuations within 1 au in Protoplanetary Disks

Protoplanetary disks are often assumed to change slowly and smoothly during planet formation. Here, we investigate the time evolution of isolated disks subject to viscosity and a disk wind. The viscosity is assumed to increase rapidly at around 900 K due to thermal ionization of alkali metals, or th...

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Hovedforfatter: John Chambers
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2024-01-01
Serier:The Astrophysical Journal
Fag:
Protoplanetary disks
Planetary system formation
Planetesimals
Planetary migration
Planet formation
Online adgang:https://doi.org/10.3847/1538-4357/ad3731
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