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Formation of the First Planetesimals via the Streaming Instability in Globally Turbulent Protoplanetary Disks?

Using self-consistent models of turbulent particle growth in an evolving protoplanetary nebula of solar composition, we find that recently proposed local metallicity and Stokes number criteria necessary for the streaming instability to generate gravitationally bound particle overdensities are genera...

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Bibliografske podrobnosti
Principais autores: Paul R. Estrada, Orkan M. Umurhan
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2023-01-01
Serija:The Astrophysical Journal
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Online dostop:https://doi.org/10.3847/1538-4357/acb7db
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