Titlebook: Dust-Gas Instabilities in Protoplanetary Disks; Toward Understanding Ryosuke Tominaga Book 2022 The Editor(s) (if applicable) and The Autho

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,Summary and?Future Prospects,here planetesimals form are not smooth profile as assumed in the classical standard theory but quite structured. Especially, dust rings and gaps have been frequently observed, which might be the key to explain dust growth toward planetesimals in protoplanetary disks. In this thesis, we investigate d

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Ryosuke TominagaHighlights new instability triggered by dust-gas friction and turbulent viscosity.Presents a new instability driven by dust coagulation in protoplanetary disks.Offers a planetesimal formation scenario

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Springer Theseshttp://image.papertrans.cn/e/image/283450.jpg

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