On the formation of planetary systems via oligarchic growth in thermally evolving viscous discs

We present N-body simulations of planetary system formation in thermally evolving, viscous disc models. The simulations incorporate type I migration (including corotation torques and their saturation), gap formation, type II migration, gas accretion on to planetary cores and gas disc dispersal throu...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2014-11, Vol.445 (1), p.479-499
Main Authors: Coleman, Gavin A. L., Nelson, Richard P.
Format: Article
Language:English
Subjects:
Accretion disks
Corotation
Discs
Disks
Extrasolar planets
Formations
Migration
Planetary systems
Simulation
Star & galaxy formation
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