Dust-Gas Instabilities in Protoplanetary Disks(Springer Theses)

原行星盘中的尘气不稳定性:了解小行星的形成

天文学史

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作      者
出  版 社
出版时间
2022年05月19日
装      帧
精装
ISBN
9789811917646
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页      码
116
开      本
9.21 x 6.14 x 0.38
语      种
英文
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图书简介
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.
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