| 書目名稱 | Dust-Gas Instabilities in Protoplanetary Disks |
| 副標(biāo)題 | Toward Understanding |
| 編輯 | Ryosuke Tominaga |
| 視頻video | http://file.papertrans.cn/284/283450/283450.mp4 |
| 概述 | Highlights 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 |
| 叢書名稱 | Springer Theses |
| 圖書封面 |  |
| 描述 | .How planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed..This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings.. |
| 出版日期 | Book 2022 |
| 關(guān)鍵詞 | Disk Evoluation; Planet Formation in Protoplanetary Disks; Secular Gravitational Instability; Hydrodyna |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-981-19-1765-3 |
| isbn_softcover | 978-981-19-1767-7 |
| isbn_ebook | 978-981-19-1765-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor |
|Archiver|手機(jī)版|小黑屋|
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