Radiative transfer in very optically thick circumstellar disks

Astronomy and Astrophysics

Volumn 497, Issue 1, 2009, Pages 155-166

  Min, M ^a   Dullemond, C P ^b   Dominik, C ^a   De Koter, A ^a,c   Hovenier, J W ^a  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UTRECHT UNIVERSITY   (Netherlands)

Author keywords

Diffusion; Radiative transfer; Stars: circumstellar matter

Indexed keywords

CIRCUMSTELLAR DISKS; COMPUTATION TIME; COMPUTATIONAL SPEED; DIFFUSION APPROXIMATIONS; DISK STRUCTURES; EFFICIENT IMPLEMENTATIONS; ENERGY DIFFUSIONS; HIGH-DENSITY REGIONS; HYDROSTATIC EQUILIBRIUMS; LOWER DENSITIES; MONTE CARLO; PARAMETER SPACES; PHOTON COUNTS; RADIATIVE TRANSFER CODES; RANDOM WALKS; STARS: CIRCUMSTELLAR MATTER; STATISTICAL NOISE; TEMPERATURE STRUCTURES; VERTICAL STRUCTURES;

DIFFUSION; DISKS (MACHINE COMPONENTS); PHOTONS; RADIATIVE TRANSFER; STARS;

DISKS (STRUCTURAL COMPONENTS);

EID: 63849286692     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811470     Document Type: Article

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