From protoplanetary disks to planet formation : Saas-Fee advanced course 45 ; Swiss Society for Astrophysics and Astronomy /: Saas-Fee advanced course 45 ; Swiss Society for Astrophysics and Astronomy. (2019)

• Record Type: Book
• Further Information: Note: Philip J. Armitage, Wilhelm Kley ; edited by Marc Audard, Michael R. Meyer, Yann Alibert.
• Authors: Armitage, Philip J, 1971-; Kley, Wilhelm
• Editors: Audard, Marc; (Astronomer), Meyer, Michael R; Alibert, Yann
• Contents: Intro; Preface; Acknowledgements; Contents; List of Figures; List of Tables; 1 Physical Processes in Protoplanetary Disks; 1.1 Preamble; 1.2 Observational Context; 1.2.1 The Classification of Young Stellar Objects; 1.2.2 Accretion Rates and Lifetimes; 1.2.3 Inferences from the Dust Continuum; 1.2.4 Molecular Line Observations; 1.2.5 Large-Scale-Structure in Disks; 1.3 Disk Structure; 1.3.1 Vertical and Radial Structure; 1.3.2 Thermal Physics; 1.3.3 Ionization Structure; 1.4 Disk Evolution; 1.4.1 The Classical Equations; 1.4.2 Boundary Conditions; 1.4.3 Viscous Heating; 1.4.4 Warped Disks 1.4.5 Disk Winds1.5 Turbulence; 1.5.1 Hydrodynamic Turbulence; 1.5.2 Self-gravity; 1.5.3 Magnetohydrodynamic Turbulence and Transport; 1.5.4 The Magnetorotational Instability; 1.5.5 Transport in the Boundary Layer; 1.6 Episodic Accretion; 1.6.1 Secular Disk Instabilities; 1.6.2 Triggered Accretion Outbursts; 1.7 Single and Collective Particle Evolution; 1.7.1 Radial Drift; 1.7.2 Vertical Settling; 1.7.3 Streaming Instability; 1.8 Structure Formation in Protoplanetary Disks; 1.8.1 Ice Lines; 1.8.2 Particle Traps; 1.8.3 Zonal Flows; 1.8.4 Vortices; 1.8.5 Rossby Wave Instability 1.9 Disk Dispersal1.9.1 Photoevaporation; 1.9.2 MHD Winds; References; 2 Planet Formation and Disk-Planet Interactions; 2.1 Introduction; 2.1.1 The Solar System; 2.1.2 Properties of the Extrasolar Planets; 2.1.3 Pathways to Planets; 2.2 From Dust to Planetesimals; 2.2.1 Study the Initial Growth Phase; 2.2.2 How to Overcome Growth Barriers; 2.2.3 Dust Concentration; 2.3 Terrestrial Planet Formation; 2.3.1 Concepts; 2.3.2 Growth to Protoplanets; 2.3.3 Assembly of the Terrestrial Planets; 2.4 The Formation of Massive Planets by Core Accretion; 2.4.1 Background; 2.4.2 The Growth to a Giant 2.4.3 The Final Mass2.4.4 Interior Structure of Planets; 2.5 Planets Formed by Gravitational Instability; 2.5.1 Background; 2.5.2 Linear Stability Analyses; 2.5.3 Fragmentation Conditions; 2.5.4 Non-linear Simulations; 2.6 Planet-Disk Interaction; 2.6.1 Basic Concepts; 2.6.2 Type I Migration; 2.6.3 Type II Migration; 2.6.4 Other Regimes of Migration; 2.6.5 Eccentricity and Inclination; 2.7 Multi-body Systems; 2.7.1 Resonances; 2.7.2 Dynamics; 2.7.3 Multi-planet Systems; 2.7.4 Circumbinary Planets; References
• Publisher Details: Berlin, Germany : Springer
• Publication Date: 2019
• Extent: 1 online resource (xxxiii, 260 pages), illustrations (some color)
• Subjects: 523.01; Disks (Astrophysics); Planets -- Origin; Disks (Astrophysics); Planets -- Origin; Electronic books; Electronic books
• Languages: English
• ISBNs: 9783662586877; 3662586878
• Related ISBNs: 9783662586860
• Notes: Note: Includes bibliographical references.; Note: Online resource; title from PDF title page (SpringerLink, viewed February 5, 2019).
• Access Rights: Legal Deposit; Only available on premises controlled by the deposit library and to one user at any one time; The Legal Deposit Libraries (Non-Print Works) Regulations (UK).
• Access Usage: Restricted: Printing from this resource is governed by The Legal Deposit Libraries (Non-Print Works) Regulations (UK) and UK copyright law currently in force.