Disk planet interactions and early evolution in young planetary systems

DOI10.1007/S10569-004-4817-3zbMath1094.70009arXivastro-ph/0412700OpenAlexW2082157475MaRDI QIDQ1776099

J. C. B. Papaloizou

Publication date: 20 May 2005

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0412700

zbMATH Keywords

MHD turbulenceaccretion disksorbital migration

Mathematics Subject Classification ID

Celestial mechanics (70F15) Astrophysical cosmology (85A40)

Uses Software

• MOCCT

Cites Work

• MOCCT: A numerical technique for astrophysical MHD

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