Effects of scattering and dust grain size on the temperature structure of protoplanetary discs: A three-layer approach

Monthly Notices of the Royal Astronomical Society

Volumn 393, Issue 4, 2009, Pages 1377-1390

  Inoue, Akio K ^a   Oka, Akinori ^b   Nakamoto, Taishi ^b  

^a OSAKA SANGYO UNIVERSITY   (Japan)

^b TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

Author keywords

Dust, extinction; Methods: analytical; Methods: numerical; Planetary systems: protoplanetary discs; Radiative transfer; Scattering

Indexed keywords

ANALYTICAL MODELS; DUST; GRAIN SIZE AND SHAPE; NUMERICAL METHODS; NUMERICAL MODELS; RADIATION; STARS;

DIFFUSE RADIATION; DUST EXTINCTIONS; GRAINSIZE; INTERIOR TEMPERATURE; ISOTROPIC SCATTERING; METHOD: NUMERICAL; METHODS:ANALYTICAL; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; PROTOPLANETARY DISKS; THREE-LAYER;

ENERGY DISSIPATION;

EID: 61349091712     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14316.x     Document Type: Article

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