Type I migration in optically thick accretion discs

Monthly Notices of the Royal Astronomical Society

Volumn 424, Issue 4, 2012, Pages 2746-2756

  Yamada, K ^a,b   Inaba, S ^b  

^a KOBE UNIVERSITY   (Japan)

^b WASEDA UNIVERSITY   (Japan)

Author keywords

Hydrodynamics; Methods: numerical; Planets and satellites: formation

Indexed keywords

EARTH (PLANET); HYDRODYNAMICS; NUMERICAL METHODS; ORBITS; SATELLITES; TEMPERATURE; TORQUE; VISCOSITY;

ACCRETION DISCS; CO-ROTATION; COOLING RATES; ENTROPY DISTRIBUTION; HIGHEST TEMPERATURE; INNER REGION; METHOD: NUMERICAL; PLANETS AND SATELLITES: FORMATION; RADIATIVE COOLING; VISCOUS HEATING;

PLANETS;

EID: 84864942294     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21375.x     Document Type: Article

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