Rapid inward migration of planets formed by gravitational instability

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 3, 2011, Pages 1971-1982

  Baruteau, Clément ^a,b   Meru, Farzana ^c,d   Paardekooper, Sijme Jan ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF EXETER   (United Kingdom)

^d UNIVERSITY OF TÜBINGEN   (Germany)

Author keywords

Accretion, accretion discs; Hydrodynamics; Methods: numerical; Planet disc interactions; Protoplanetary discs; Turbulence

Indexed keywords

ASPECT RATIO; GRAVITATION; HYDRODYNAMICS; NUMERICAL METHODS; ORBITS; STARS; STOCHASTIC SYSTEMS;

ACCRETION: ACCRETION DISKS; EXO-PLANETS; FORMATION MECHANISM; GRAVITATIONAL INSTABILITY; HOST-STARS; METHOD: NUMERICAL; PLANET FORMATION; PLANET-DISK INTERACTIONS; PROTOPLANETARY DISKS; STAR-LIKE;

PLANETS;

EID: 80052615683     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19172.x     Document Type: Article

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