Pileups and Migration Rates for Planets in Low-mass Disks

We investigate how planets interact with viscous accretion disks, in the limit that the disk is sufficiently low mass that the planet migrates more slowly than the disk material. In that case, the disk's surface density profile is determined by the disk being in viscous steady state (VSS) while...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	The Astrophysical journal 2020-03, Vol.891 (2), p.108
Hauptverfasser:	Dempsey, Adam M., Lee, Wing-Kit, Lithwick, Yoram
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astrophysics Boundary conditions Circumstellar disks Computer simulation One dimensional models Planet formation Planetary orbits Planets Protoplanetary disks Protoplanets Simulation Viscosity
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!