The interaction of giant planets with a disc with MHD turbulence - III. Flow morphology and conditions for gap formation in local and global simulations

Monthly Notices of the Royal Astronomical Society

Volumn 350, Issue 3, 2004, Pages 829-848

  Papaloizou, John C B ^a   Nelson, Richard P ^a   Snellgrove, Mark D ^a  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Accretion, accretion discs; Instabilities; MHD; Planetary systems: formation; Planetary systems: protoplanetary discs; Turbulence

Indexed keywords

MAGNETOHYDRODYNAMICS; ORBITS; TURBULENCE; WAKES;

ACCRETION: ACCRETION DISKS; CONDITION; GAP FORMATION; GIANT PLANETS; GLOBAL SIMULATION; MAGNETIC-FIELD; MAGNETOHYDRODYNAMIC TURBULENCE; PLANETARY SYSTEMS:FORMATION; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; PROTOPLANETS;

SHEARING;

EID: 2642532568     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07566.x     Document Type: Article

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