Three-dimensional calculations of high- And low-mass planets embedded in protoplanetary discs

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 1, 2003, Pages 213-229

  Bate, M R ^a   Lubow, S H ^b   Ogilvie, G I ^c   Miller, K A ^d  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b STScI   (United States)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d Bldg 142   (United States)

Author keywords

Accretion, accretion discs; Hydrodynamics; Planetary systems: Formation; Planetary systems: Protoplanetary discs; Planets and satellites: Formation

Indexed keywords

EARTH (PLANET); FLOW OF GASES; FLOW PATTERNS; ORBITS; PLANETS; SATELLITES;

ACCRETION RATE; ACCRETION: ACCRETION DISKS; LOW-MASS; MIGRATION TIME; NON LINEAR; PLANETARY SYSTEMS:FORMATION; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; THREE-DIMENSIONAL CALCULATIONS;

HYDRODYNAMICS;

EID: 0042116685     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06406.x     Document Type: Article

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