Three Dimensional Radiative Transfer

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dc.creatorAbel, Tom
dc.date2000-05-09
dc.date.accessioned2026-07-07T01:53:28Z
dc.date.available2026-07-07T01:53:28Z
dc.descriptionRadiative Transfer (RT) effects play a crucial role in the thermal history of the intergalactic medium. Here I discuss recent advances in the development of numerical methods that introduce RT to cosmological hydrodynamics. These methods can also readily be applied to time dependent problems on interstellar and galactic scales.
dc.description5 pages, 2 figures, To appear in "Astrophysical Plasmas: Theory, Codes & Models", Eds. J. Arthur and J. Franco, Rev. Mex. A. & A., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0005191
dc.identifierhttp://arxiv.org/abs/astro-ph/0005191
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/980
dc.subjectAstrophysics
dc.titleThree Dimensional Radiative Transfer
dc.typetext

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