Numerical simulations of type III planetary migration - II. Inward migration of massive planets

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 1, 2008, Pages 179-198

  Peplinski A ^a   Artymowicz, P ^b   Mellema, G ^a  

^a STOCKHOLM UNIVERSITY   (Sweden)

^b UNIVERSITY OF TORONTO   (Canada)

Author keywords

Accretion, accretion discs; Hydrodynamics; Methods: numerical; Planets and satellites: formation

Indexed keywords

NUMERICAL METHODS; ORBITS; SATELLITES;

ACCRETION: ACCRETION DISKS; ADAPTIVE MESH REFINEMENT; CO-ROTATION; INITIAL CONDITIONS; JUPITERS; KEYS PARAMETERS; METHOD: NUMERICAL; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; TWO-DIMENSIONAL;

PLANETS;

EID: 42449119851     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13046.x     Document Type: Article

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