2004•Unpublished venueRequires access

The Two-Fluid Analysis of the Kelvin-Helmholtz Instability in the Dust Layer of a Protoplanetary Disk: A Possible Path to the Planetesimal Formation Through the Gravitational Instability

Shugo Michikoshi, Shu‐ichiro Inutsuka

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Key concepts: Planetesimal, Gravitational instability, Instability, Physics, Protoplanetary disk, Planet, Astrobiology, Streaming instability

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The Two-Fluid Analysis of the Kelvin-Helmholtz Instability in the Dust Layer of a Protoplanetary Disk: A Possible Path to the Planetesimal Formation Through the Gravitational Instability — Research Paper | ScholarLens