The importance of photosphere cooling in simulations of gravitational instability in the inner regions of protostellar discs

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 2, 2011, Pages 913-929

  Rogers, Patrick D ^a   Wadsley, James ^a  

^a MCMASTER UNIVERSITY   (Canada)

Author keywords

Hydrodynamics; Methods: numerical; Planetary systems; Protoplanetary discs; Radiative transfer

Indexed keywords

COOLING; HYDRODYNAMICS; NUMERICAL METHODS; PLANETS; STARS;

BOUNDARY TREATMENT; COOLING RATES; GIANT PLANETS; GRAVITATIONAL INSTABILITY; INNER REGION; METHOD: NUMERICAL; PLANETARY SYSTEM; PROTOPLANETARY DISKS; PROTOSTELLAR DISKS; RELAXATION TEST;

RADIATIVE TRANSFER;

EID: 79958116578     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18523.x     Document Type: Article

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