Radiative cooling in numerical astrophysics: the need for adaptive mesh refinement

DOI10.1016/j.compfluid.2010.10.022zbMath1271.76202arXiv1011.2610OpenAlexW2077963378WikidataQ60718160 ScholiaQ60718160MaRDI QIDQ365221

Allard Jan van Marle, Rony Keppens

Publication date: 4 September 2013

Published in: Computers and Fluids (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1011.2610

zbMATH Keywords

circumstellar envelopescomputational techniques: fluid dynamicsradiative recombinationradiative transfer in astrophysicsstellar winds

Mathematics Subject Classification ID

Finite volume methods applied to problems in fluid mechanics (76M12) Gas dynamics (general theory) (76N15) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Parallel, grid-adaptive approaches for relativistic hydro- and magnetohydrodynamics

Cites Work

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