Dust-Gas Instabilities in Protoplanetary Disks

Toward Understanding Planetesimal Formation de

Éditeur :

Springer


Collection :

Springer Theses

Paru le : 2022-04-25

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Description

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.
Pages
116 pages
Collection
Springer Theses
Parution
2022-04-25
Marque
Springer
EAN papier
9789811917646
EAN PDF
9789811917653

Informations sur l'ebook
Nombre pages copiables
1
Nombre pages imprimables
11
Taille du fichier
3697 Ko
Prix
147,69 €
EAN EPUB
9789811917653

Informations sur l'ebook
Nombre pages copiables
1
Nombre pages imprimables
11
Taille du fichier
14008 Ko
Prix
147,69 €