Gravitational interaction between a planet and an optically thin disc

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 3, 2003, Pages 915-923

  Morohoshi, K ^a,b   Tanaka, H ^a  

^a TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^b TOYOTA MOTOR CORPORATION   (Japan)

Author keywords

Hydrodynamics; Methods: numerical; Planetary systems: formation; Planetary systems: protoplanetary discs; Radiative transfer

Indexed keywords

COOLING; ENERGY TRANSFER; GRAIN GROWTH; NUMERICAL METHODS; RADIATIVE TRANSFER; TORQUE;

DUST OPACITY; GRAVITATIONAL INTERACTION; METHOD: NUMERICAL; OPTICAL THICKNESS; PLANETARY SYSTEMS:FORMATION; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; PROTOPLANETARY DISKS; RADIATIVE COOLING; RADIATIVE ENERGY TRANSFER; THIN DISK;

PLANETS;

EID: 0347528579     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2003.07140.x     Document Type: Article

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