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Journal of computational physics, ISSN 0021-9991, 2012, Volume 231, Issue 3, pp. 759 - 794
Journal Article
The Astrophysical journal. Supplement series, ISSN 1538-4365, 2011, Volume 194, Issue 2, p. 23
Journal Article
Journal of Computational Physics, ISSN 0021-9991, 02/2017, Volume 330, Issue C, pp. 924 - 942
We present a highly-parallel multi-frequency hybrid radiation hydrodynamics algorithm that combines a spatially-adaptive long characteristics method for the radiation field from point sources... 
Hydrodynamics | Radiative transfer | Adaptive mesh refinement | Long characteristics | Parallelization | MOLECULAR CLOUDS | RESOLUTION | STAR-FORMATION SIMULATIONS | EQUATIONS | PHYSICS, MATHEMATICAL | SCHEME | PRESSURE | TRANSPORT | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | MESH REFINEMENT | DIFFUSION | HII-REGIONS | Algorithms | Fluid dynamics | Analysis | Methods | Astronomy | Radiation
Journal Article
Journal Article
2004, ISBN 9780521833097, 369
This broad treatment provides an accessible introduction to the theory and the large-scale simulation methods currently used in radiation hydrodynamics... 
Radiative transfer | Physics | Hydrodynamics | Astrophysics
Book
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 543, p. A60
.... Many previous simulations of gravitational collapse of a cold gas cloud followed by the formation of a protostellar core have used a grey treatment of radiative transfer coupled to the hydrodynamics... 
Hydrodynamics | Radiative transfer | Stars: formation | Methods: numerical | MEAN OPACITIES | radiative transfer | INTERSTELLAR DUST | STAR-FORMATION | hydrodynamics | MODEL | methods: numerical | SMOOTHED PARTICLE HYDRODYNAMICS | ACCRETION SHOCK | stars: formation | CODE | ASTRONOMY & ASTROPHYSICS | MOLECULAR CLOUD CORES | EQUATION | Physics - Solar and Stellar Astrophysics | Galactic Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2015, Volume 574, p. A81
.... However, protoplanetary disks evolve with time, and so to understand disk evolution and by association, disk structure, one should solve the combined and time-dependent equations of radiation hydrodynamics. Methods... 
Hydrodynamics | Radiative transfer | Protoplanetary disks | Accretion accretion disks | Methods: numerical | accretion, accretion disks | radiative transfer | FLUX-LIMITED DIFFUSION | STAR-FORMATION | hydrodynamics | SHOCK HYDRODYNAMICS | MAGNETOHYDRODYNAMICS | methods: numerical | DISTRIBUTIONS | TRANSPORT | CODE | ASTRONOMY & ASTROPHYSICS | CIRCUMSTELLAR DISKS | protoplanetary disks | SIMULATIONS | FLOWS | Protoplanets | Fluid dynamics | Planet formation | Mathematical analysis | Fluid flow | Irradiation | Evolution
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 2013, Volume 436, Issue 3, pp. 2188 - 2231
Journal Article
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2009, Volume 506, Issue 3, pp. 1351 - 1365
Journal Article