Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Kuiper, R ^a,c   Klahr, H ^a   Dullemond, C ^a   Kley, W ^b   Henning, T ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b UNIVERSITY OF TÜBINGEN   (Germany)

^c University of Heidelberg   (Germany)

Author keywords

Accretion, accretion disks; Circumstellar matter; Hydrodynamics; Methods: numerical; Radiative transfer; Stars: formation

Indexed keywords

ACCRETION , ACCRETION DISKS; ACCRETION DISKS; BENCHMARK TESTS; CENTRAL SOURCE; CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; DIFFUSION LIMITS; DISTRIBUTED MEMORY MACHINES; DUST GRAINS; DUST OPACITY; FIRST ORDER; FREQUENCY DEPENDENCE; FREQUENCY DEPENDENT; HIGH-ORDER; HYDRODYNAMICS SIMULATIONS; MASSIVE STARS; MESSAGE PASSING INTERFACE; METHODS: NUMERICAL; MONTE CARLO; OPTICAL DEPTH; PARALLEL SPEEDUPS; PRESTELLAR CORES; RADIATION HYDRODYNAMICS; RADIATION TRANSPORT; RADIATIVE FORCES; RADIATIVE TRANSFER CODES; SPATIAL CONFIGURATION; STARS: FORMATION; STELLAR IRRADIATION; TRANSITION REGIONS;

DIFFUSION; DISKS (MACHINE COMPONENTS); DUST; FLUID DYNAMICS; IRRADIATION; MAGNETOHYDRODYNAMICS; MESSAGE PASSING; NUMERICAL METHODS; RADIATIVE TRANSFER; THERMODYNAMICS; THREE DIMENSIONAL;

STARS;

EID: 79952845828     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912355     Document Type: Article

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